R     And    SiO maser.
S     And    SN (NGC 224).
W     And    SiO maser.
Z     And    Outbursts, average cycle 8400d. Porb = 758.8d, it reveals
Z     And    itself in photometry during the low state. A quasi-period, P1,
Z     And    about 656d is present during the outbursts. The beat period
Z     And    between Porb and P1, about 5500d, is also found in the
Z     And    photometric data.
RS    And    H2O maser.
RT    And    Min II = 9.28. P varies, current elements are given.
RU    And    P varies strongly.
RX    And    Porb = 0.209893d.
RY    And    OH, H2O maser.
SS    And    P2 = 650d, P3 = 3800d.
SU    And    VB A (B 12.77m, F0V:, 15").
SV    And    SiO maser.
SW    And    [Fe/H] = -0.24. P varies, current elements are given.
SW    And    According to [N0037], Max = 2435249.25744 + 0.442270491d*E -
SW    And    1.032 x 10^{-10}E*E.
SY    And    d = 0.027P.
TT    And    Min II = 11.6.
TW    And    d = 0.020P, Min II = 9.13. P varies, current elements are given.
TX    And    Recent observations in the AAVSO database suggest type LB.
UU    And    The depth of MinII is 0.2m R. P varies, current elements are
UU    And    given.
VX    And    The mean brightness varies with P = 904d.
WW    And    The depth of MinII is 0.16m.
WX    And    d = 0.03P. P varies, current elements are given.
WY    And    [Fe/H] = -1.0.
WZ    And    Min II = 11.61. P varies, current elements are given. Min II 11.61.
XX    And    P varies, current elements are given. [Fe/H] = -1.94.
XX    And    Blazhko effect with a 36-day period [03111].
XY    And    [Fe/H] = -0.92.
XZ    And    P varies in a complex manner, current elements are given.
ZZ    And    [Fe/H] = -1.58.
AA    And    Min II = 10.6.
AB    And    Min II = 10.32. P varies, current elements are given. The light curve shape
AB    And    varies.
AC    And    A triple-mode pulsator. The table gives the light elements for
AC    And    the fundamental-mode pulsations. First overtone: Max =
AC    And    2428009.45 + 0.5251342d*E; second overtone: Max =
AC    And    2428009.69 + 0.4210572d*E. [Fe/H] = -1.16.
AD    And    The depth of Min II is 0.58m. P varies, current elements are
AD    And    given.
AE    And    In the M31 galaxy.
AF    And    In the M31 galaxy.
AG    And    The data in [75119] refer to a different star. The data in
AG    And    [08296] probably refer to a different star.
AM    And    VB A (B 14.7m 17" sf).
AN    And    Min II = 6.05.
AP    And    Min II = 11.8.
AQ    And    Secondary period 346d.
AR    And    Porb = 0.16302d.
AT    And    [Fe/H] = -1.18.
AW    And    Identified by its number from the Harvard - Groningen
AW    And    Durchmusterung quoted in [01992], in 1 degree of declination
AW    And    from the position published by the discoverer. Not red,
AW    And    apparently does not vary in modern automatic surveys.
BD    And    Min II = 11.4. P varies, current elements are given.
BK    And    [Fe/H] = -0.08.
BL    And    The depth of Min II is 0.32m.
BU    And    H2O maser.
BX    And    Min II = 9.12. ADS 1671 A (B 10.86m, 20", 59deg). P varies, current elements
BX    And    are given.
CC    And    Multiperiodic.
CD    And    Min II = 10.4.
CE    And    H2O maser.
CG    And    The elements in the Table correspond to maximum U-band light.
CG    And    During some seasons, short-period variations with a period
CG    And    about 125 min and an amplitude up to several hundredths of a
CG    And    magnitude were observed. In 1973, periods of 0.09325d and
CG    And    0.06737d were detected.
CI    And    [Fe/H] = -0.69.
CN    And    Min II = 9.90. P varies, quadratic term -9.8*10^{-11}*E*E.
CO    And    d = 0.06P:.
CP    And    d = 0.01P:. P varies?
CU    And    d > 0.034P. P varies?
DI    And    An unusual light curve with a secondary maximum.
DK    And    Min II = 13.1.
DL    And    In the region of the open cluster NGC 7686.
DO    And    Min II = 12.9.
DQ    And    [M/H] = 0.00.
DR    And    [Fe/H] = -1.48. P varies, current elements are given. Blazhko
DR    And    effect with a period about 57d is possible [N0053].
DS    And    d = 0.04P, Min II = 10.71. In the open cluster NGC 752. dII = 0.07P.
DU    And    [Fe/H] = -2.11.
DX    And    Porb = 0.440502d.
EG    And    Porb = 482.57d. The light curve is modulated with a double wave
EG    And    during the orbital period.
EL    And    Min II = 13.7. A twice shorter period is possible.
EP    And    The depth of Min II is 0.60m. P varies, current elements are
EP    And    given.
ET    And    SB1, Porb = 48.304d.
EU    And    H2O maser.
EX    And    Min II = 13.0. No evidence for the secondary minimum being displaced, as
EX    And    claimed in [04335], in recent CCD data. P varies?
EY    And    OH, H2O, SiO maser.
FF    And    VB A (B 10.53m V, 7", 295deg). SB2, Porb = 2.170304d.
FF    And    BY-type variations: 10.35m - 10.42m V outside flares,
FF    And    P = 2.170d [5230].
FL    And    d = 0.02P.
FO    And    Porb = 0.07161d. Superhumps: P = 0.07411d [N0067].
FV    And    P varies?
GH    And    Min II = 14.1.
GK    And    Min II = 11.5. P varies?
GN    And    ADS 409 A (B 13.1m, 2", 6deg, 1948).
GP    And    VB A (B 12.50m, 11"). P varies, quadratic term
GP    And    +5.20d*10^{-13}E*E.
GQ    And    ADS 246 B (A = GX And). 11.04m - 11.10m V outside flares
GQ    And    [08313].
GX    And    ADS 246 A (B = GQ And).
GY    And    SB1, P = 272.88d.
GZ    And    Min II = 11.58. ADS 1693 A (B 11.13m, 8", 31deg, 1894; C 11.91m, 14", 200deg,
GZ    And    1908; D 12.65m, 24", 285deg, 1908). P varies, current elements
GZ    And    are given.
HN    And    SB1, P = 106.3334d. From Hipparcos data, a photometric period
HN    And    of 1.7237d (instead of 69.92d) was suggested in [N0078].
HN    And    However, it does not represent the observations from [06992],
HN    And    where the derived period was 69.5d.
HR    And    d = 0.05P.
HS    And    P varies, current elements are given.
HT    And    In the region of the M 31 galaxy.
HU    And    Min II = 17.2.
HY    And    In the region of the M 31 galaxy.
HZ    And    P > 100d. Red.
IK    And    In the region of the M 31 galaxy.
IL    And    d = 0.02P.
IM    And    Min II = 18.8.
IO    And    In the region of the M 31 galaxy.
IP    And    d = 0.02P:.
KM    And    According to [69005], cst, 14.8m pg.
KP    And    The depth of Min II is 0.1m R.
KV    And    Superhumps: P = 0.07434d [N0087].
KX    And    SB2 (Porb = 38.908d). Porb reveals itself in seasonal light
KX    And    curves.
KZ    And    ADS 16557 B (A 7.2m; B 16", 256deg, 1984). SB2,
KZ    And    Porb = 3.032867d.
LL    And    Porb = 0.055055d.
LM    And    Min II = 12.7. VB (QY And 14" np).
LN    And    ADS 16472 (B A1V, 9.88m, 7", 40 deg).
LO    And    Min II = 11.7. P varies, current elements are given.
LQ    And    SB1, Porb = 7.413d.
LR    And    Min II = 7.14. Epoch of Max is given. P varies, quadratic term
LR    And    +3.379*10^{-9}*E*E.
LS    And    In the region of the M 31 galaxy.
LT    And    In the region of the M 31 galaxy.
LV    And    [Fe/H] = -1.55.
LY    And    Min II = 14.6.
LZ    And    Min II = 17.7.
MN    And    Min II = 15.5.
MP    And    [Fe/H] = -1.62.
MR    And    [Fe/H] = -1.26.
MS    And    Min II = 16.3.
MT    And    Min II = 15.3.
MU    And    [Fe/H] = -1.57.
MV    And    [Fe/H] = -1.78.
MW    And    Min II = 15.5.
MX    And    [Fe/H] = -1.50.
MY    And    [Fe/H] = -1.32.
MZ    And    Min II = 15.6.
NN    And    [Fe/H] = -1.35.
NO    And    [Fe/H] = -1.67.
NQ    And    [Fe/H] = -1.38.
NZ    And    Min II = 15.1.
OR    And    Porb = 0.1359d.
OT    And    Min II = 7.62. MinII - MinI = 0.52P.
OV    And    ADS 284 B (A Sp G, 7.5" p; several additional fainter
OV    And    companions).
PQ    And    Rare outbursts in 1938, 1967, 1988. Porb = 0.071d.
PT    And    In the region of the M 31 galaxy.
PU    And    Min II = 24.4. In the region of the M 31 galaxy.
PX    And    The elements are for eclipses. The amplitude of the eclipses
PX    And    is about 0.5m.
PY    And    SB, P = 399.6d.
QR    And    The elements are for eclipses.
QS    And    Min II = 17.07.
QU    And    SB1.
QW    And    The depth of MinII is 0.44m.
QX    And    Min II = 11.49. In the open cluster NGC 752. P varies?
QY    And    VB (LM And 14" sf). Variations only due to LM And are seen in
QY    And    ROTSE/NSVS data for combined light.
QZ    And    VB A (B 14" np).
V0336 And    VB A (B 20" sp).
V0337 And    VB A (B 14.0m, 15" nf).
V0342 And    Min II = 7.70. VB (A 7.86m, B 9.21m, 5", 82deg, 1991).
V0348 And    ADS 197 (B 7.5m V, 0.2", 42deg, 1957).
V0355 And    Min II = 7.9. ADS 616 (A 7.92m Hp, F5; B 9.08m Hp, 1.4", 5.5deg, 1991).
V0357 And    Min II = 6.7.
V0361 And    ADS 948 (A 7.84m, F0; B 11.65m, 3", 249deg, 1991).
V0363 And    Min II = 9.34.
V0369 And    VB (9.5m V + 9.5m V, 0".1, 128deg, 1986.9).
V0371 And    VB (ADS 1613AB: A 8.7m V, B 8.9m V, 0.2". 358deg, 1997;
V0371 And    C 11.5m V, 0.8", 261deg, 1958).
V0372 And    Min II = 9.37.
V0376 And    Min II = 7.96.
V0382 And    Min II = 9.24.
V0392 And    Min II = 9.41. VB (A 9.3m Hp; B 11.5m Hp, 2", 75deg, 1991).
V0393 And    P = 0.223880d is suggested in [HIP], the light curve has a
V0393 And    large scatter.
V0395 And    Min II = 7.61. ADS 16965 (A 7.6m V; B 9.8m V, 6", 103deg, 1991).
V0404 And    Min II = 10.8.
V0406 And    Min II = 9.39.
V0411 And    Min II = 15.3.
V0412 And    Min II = 12.35.
V0413 And    d = 0.01P. ADS 17087 (B 12.5m V, 5", 181deg, 1907).
V0419 And    ADS 1672 (B 10.0m V, 6", 254deg, 1991).
V0420 And    VB A (B 15.0m pg, 12" np).
V0422 And    Min II = 13.7.
V0428 And    SB1, Porb = 576d.
V0429 And    Multiperiodic, P1 = 195s.
V0440 And    Min II = 12.90.
V0441 And    Min II = 14.25.
V0444 And    Min II = 13.70.
V0446 And    A chromospherically active giant, photometric variations with
V0446 And    the rotation period.
V0449 And    Min II = 12.8.
V0452 And    Min II = 14.3.
V0467 And    Min II = 15.52.
V0468 And    Min II = 11.54.
V0469 And    Min II = 15.5.
V0472 And    Min II = 13.5.
V0473 And    Min II = 14.15.
V0474 And    Min II = 13.8.
V0477 And    Min II = 13.95.
V0478 And    Multiperiodic.
V0480 And    Min II = 13.0.
V0482 And    Min II = 11.45.
V0483 And    Min II = 12.2.
V0484 And    Min II = 13.28.
V0485 And    Min II = 11.22.
V0487 And    Min II = 11.74.
V0488 And    Min II = 12.65 :.
V0489 And    Min II = 12.7.
V0490 And    Min II = 15.1.
V0496 And    Min II = 12.6 :. P varies, current elements are given.
V0497 And    Min II = 15.3.
V0498 And    VB B (A 10.0mV; B 10.1mV, 22", 139deg, 2005). Combined brightness tabulated.
V0502 And    Min II = 14.15. P = 0.2750d is not excluded.
V0504 And    Min II = 13.6.
V0505 And    Min II = 14.6.
V0506 And    Min II = 14.2.
V0508 And    Min II = 12.4.
V0510 And    Min II = 14.35.
V0512 And    Min II = 11.95.
V0513 And    Min II = 12.9.
V0514 And    Min II = 14.15.
V0517 And    Min II = 13.6 :.
V0518 And    Min II = 13.85.
V0521 And    Multiperiodic.
V0522 And    Min II = 13.94. MinII - MinI = 0.484P.
V0523 And    Min II = 12.35.
V0525 And    Min II = 11.5.
V0526 And    Min II = 14.6.
V0527 And    Min II = 11.05.
V0529 And    Multiperiodic. The largest-amplitude Delta Scuti period is 0.11876d. VB A (B 13.4mV, 16", 166deg, 1998).
V0530 And    Min II = 13.0.
V0531 And    Min II = 11.55.
V0532 And    Min II = 13.75 :.
V0533 And    Min II = 14.05.
V0534 And    Min II = 14.6.
V0536 And    Min II = 14.6. Type RRC with a twice shorter period is possible.
V0537 And    Min II = 11.65.
V0538 And    Min II = 14.2.
V0541 And    Min II = 12.70.
V0543 And    Min II = 11.15.
V0546 And    Min II = 11.76.
V0547 And    Min II = 11.74.
V0549 And    Min II = 14.4.
V0552 And    Min II = 17.36.
V0553 And    Min II = 17.52.
V0554 And    Min II = 16.72.
V0555 And    Min II = 14.57.
V0556 And    Min II = 14.70.
V0557 And    Min II = 14.8.
V0558 And    Min II = 15.99.
V0559 And    Min II = 16.17.
V0560 And    Min II = 14.23. O'Connell effect.
V0561 And    Min II = 16.38.
V0563 And    Min II = 14.0.
V0564 And    Min II = 14.06.
V0565 And    Min II = 12.25.
V0566 And    Min II = 11.25.
V0567 And    Min II = 11.8.
V0568 And    Min II = 14.4.
V0571 And    Min II = 14.1.
V0575 And    Min II = 12.35.
V0604 And    The coordinates in [598] are wrong.
alf   And    SB2 (P = 96.7041d). VB (interferometric, a = 0.024").
alf   And    Photometric variability could not be confirmed in [N0111].
zet   And    For regular ellipsoidal variations, the depth of minima are
zet   And    about 0.07m.
lam   And    The tabulated elements are for brightness minima in 1996 - 2002.
lam   And    SB1 (P = 20.5212d).
omi   And    Multiple (AB 0.3", period much longer than 100d; Aa 0.05";
omi   And    B SB2, P = 33.08d). Several shell events were observed.
omi   And    Periodic variations with varying amplitude (up to 0.1m):
omi   And    double wave, MinI = 2429981.250 + 1.571272d*E [N0114]. A number
omi   And    of different photometric and spectroscopic periods were also
omi   And    reported.
S     Ant    Min II = 6.80.
T     Ant    [A/H] = -0.0. P var, nonlinear elements: Max = 2436120.756
T     Ant    + 5.897915d*E + 4.80d*10^{-8}E^2 [00027].
V     Ant    OH, H_2O, SiO maser.
Y     Ant    Min II = 10.63.
SW    Ant    Min II = 13.7.
SZ    Ant    From photometry in [00002], about 12.3m V, const? [00000].
TU    Ant    From photometry in [00002], about 10.6m V, const? [00000].
UU    Ant    Min II = 12.1.
VV    Ant    Min II = 13.1.
WX    Ant    Min II = 11.6.
WY    Ant    [Fe/H] = -1.48. P var, nonlinear elements: Max =
WY    Ant    2439139.40 + 0.574330174d*E + 4.820d*10^{-10}E^2 [00029].
WZ    Ant    Min II = 12.1.
XX    Ant    Min II = 9.23.
YZ    Ant    Min II = 10.56.
AG    Ant    [Fe/H] = -4.8. A post-AGB star. SB1. Brightness variations with
AG    Ant    the orbital period probably due to variations of circumstellar
AG    Ant    extinction.
AI    Ant    Slow variations with Prot (see Table), oscillations with P about
AI    Ant    15 minutes, several frequencies.
AN    Ant    Min II = 8.26.
BN    Ant    Identification according to [064]. Not CPD-38 03763 (identification suggested in [091]).
BU    Ant    VB A (B 11.72m, 27", 36deg, 2000).
BV    Ant    MinII - MinI = 0.56P.
BW    Ant    Porb = 0.030263d.
BY    Ant    Min II = 9.26.
BZ    Ant    VB B (A 5.56m, NSV 04876; AB 11", 226deg, 1999).
CC    Ant    Min II = 7.78.
CD    Ant    Min II = 10.63.
RS    Aps    VB A (A 15.1mV; B 15.5mV, 6", 139deg, 1999).
TY    Aps    Blazhko effect? [Fe/H] = -0.95.
UW    Aps    VB A (A 15.4mV, B 15.7mV; AB 9", 147deg, 2000).
VX    Aps    [Fe/H] = -1.44.
YZ    Aps    VB (14.2m, 14.6m, 8", 207deg, 2000). The southern component varies?
AB    Aps    [Fe/H] = -1.30.
BE    Aps    OH maser.
BM    Aps    VB A (B 12.2mR, 18", 137deg, 2000). The tabulated magnitude in maximum is influenced by the companion.
BS    Aps    [Fe/H] = -1.33.
CE    Aps    VB A (B 13m, 14", 125deg; C 14m, 199deg, 2000).
CK    Aps    [Fe/H] = -1.49.
CP    Aps    VB A (B 15.2m, 9", 289deg, 2000). It is not quite clear which of the components varies.
CZ    Aps    SiO maser.
DF    Aps    VB A (B 15.5mpg, 14", 308deg, 2000).
DI    Aps    Blazhko effect? [Fe/H] = -1.60.
DZ    Aps    Blazhko effect.
EL    Aps    [Fe/H] = -1.56.
ER    Aps    [Fe/H] = -1.39.
EX    Aps    [Fe/H] = -0.81.
GO    Aps    Type RR is not excluded.
IP    Aps    VB B (A 14.5mpg, B 14.7mpg; AB 10", 140deg, 2000).
IZ    Aps    VB B (A 15.4mpg, B 16.4mpg; AB 8", 300deg, 2000).
LM    Aps    Type RV is also possible.
LO    Aps    O'Connell effect.
LU    Aps    [Fe/H] = -2.06.
MY    Aps    L19-2. Multiperiodic, main stable modes: 192.6s and 113.8s.
OZ    Aps    A twice longer period is not excluded.
PQ    Aps    In the region of the globular cluster IC 4499; cluster non-member.
PV    Aps    MinII - MinI = 0.75P.
QX    Aps    Superposed variations with P = 74d: and an amplitude about 1m.
V0347 Aps    VB A (A 13.5m; B 15.1m, 10", 79deg, 2000; C 5", 321deg, 2000). The tabulated amplitude was affected by the companions.
kap 1 Aps    SB. VB A (B 11.27m, 27", 255deg, 2000).
R     Aqr    P varies, current elements are given. SiO, OH, H2O maser.
R     Aqr    Porb = 44 years? In a nebula, has a jet. During certain time
R     Aqr    intervals several years long, too faint maxima and/or too bright
R     Aqr    minima, with the total range within two magnitudes.
V     Aqr    H2O maser. Biperiodic, P1 is given in the Table, P0 = 689d.
W     Aqr    SiO maser.
RX    Aqr    H2O maser.
RY    Aqr    Min II = 8.92. P varies, current elements are given. ADS 14862 A (B 12.65m, 4",
RY    Aqr    238deg, 1899).
ST    Aqr    Min II = 9.37. P varies, current elements are given.
SU    Aqr    Min II = 9.74. ADS 16318 A (B 10.7m, 5", 143deg, 1926). The range given is for
SU    Aqr    the combined brightness.
SW    Aqr    [Fe/H] = -1.63.
SX    Aqr    [Fe/H] = -1.87.
TT    Aqr    VB A (B 15.0m, 3", 135deg, 1830).
TZ    Aqr    [Fe/H] = -1.24.
UU    Aqr    The elements are for eclipses, about 1.3m V deep. Strong
UU    Aqr    nova-like variations (see [N0116]).
VY    Aqr    Rare outbursts. Porb = 0.06309d.
XX    Aqr    OH maser.
XZ    Aqr    P varies, current elements are given. The depth of MinII is
XZ    Aqr    about 0.2m V.
YZ    Aqr    [Fe/H] = -1.55.
AA    Aqr    [Fe/H] = -2.09.
AE    Aqr    Porb = 0.4116556d. Short flares, flickering. Ellipsoidal
AE    Aqr    variations with Porb and an amplitude of 0.3m V [N0118].
AE    Aqr    Optical oscillations with P = 33.076737s [08675] and an
AE    Aqr    amplitude up to 0.02m are considered the spin period of the
AE    Aqr    white dwarf, a twice shorter period was also reported.
AM    Aqr    Min II = 13.6.
AO    Aqr    Min II = 11.65.
AT    Aqr    Min II = 13.9.
AU    Aqr    Min II = 13.2.
AX    Aqr    [Fe/H] = -1.88. P varies, current elements are given.
AY    Aqr    Min II = 14.3.
BB    Aqr    [Fe/H] = -1.55.
BG    Aqr    [Fe/H] = -1.51.
BH    Aqr    [Fe/H] = -1.80. P varies?
BI    Aqr    Min II = 12.4.
BN    Aqr    [Fe/H] = -1.33. P varies, current elements are given.
BO    Aqr    [Fe/H] = -1.80. P varies? Current elements are given.
BQ    Aqr    d = 0.05P:, Min II = 10.9. P varies?
BR    Aqr    [Fe/H] = -0.74. P varies?
BS    Aqr    P varies? Current elements are given.
BT    Aqr    [Fe/H] = -0.29. P varies, current elements are given.
BV    Aqr    [Fe/H] = -1.18. P varies?
BW    Aqr    Min II = 10.86. DII = 0.06P, Min II - Min I = 0.478P (1983. Apsidal motion.
BX    Aqr    Min II = 12.2. P varies, current elements are given.
CD    Aqr    Min II = 11.0.
CF    Aqr    [Fe/H] = -1.03.
CH    Aqr    [Fe/H] = -1.61.
CK    Aqr    Min II = 13.38.
CP    Aqr    [Fe/H] = -0.77.
CR    Aqr    Min II = 13.9.
CV    Aqr    Minor planet (52) Europa.
CW    Aqr    Min II = 10.83.
CX    Aqr    Min II = 10.90. P varies, current elements are given.
CY    Aqr    [Fe/H] = -1.65. P varies, current elements are given.
CZ    Aqr    Min II = 11.00.
DD    Aqr    P varies, current elements are given.
DN    Aqr    [Fe/H] = -1.66.
DO    Aqr    P varies.
DS    Aqr    [Fe/H] = -1.1.
DU    Aqr    The minor planet (57) Mnemosyne. The data in [00797] must refer
DU    Aqr    to another star.
DV    Aqr    Min II = 6.1. A shell spectral episode was reported in [08062].
DX    Aqr    Min II = 6.55. ADS 15562 B (A 7.36m, K0III; B 4.0", 332deg, 1991). The range
DX    Aqr    in the Table is for combined brightness.
DY    Aqr    Min II = 10.32.
EE    Aqr    Min II = 8.12.
EF    Aqr    Min II = 10.11.
EI    Aqr    Min II = 11.6.
EK    Aqr    Min II = 11.23.
EL    Aqr    Min II = 10.71.
EP    Aqr    SiO, H2O maser.
EX    Aqr    Min II = 11.8.
EZ    Aqr    VB (AB a = 0.36", P = 2.20 years; A SB, P = 3.786516d).
EZ    Aqr    BY-type variations: Prot is about 4d [N0120].
FF    Aqr    d = 0.059P. The amplitude of the distortion wave is 0.22m U.
FG    Aqr    VB A (B = NSV 14102, 8", 212deg, 1982.66).
FI    Aqr    P = 4.659d or 4.719d not excluded.
FK    Aqr    BDS 11854 A (B = FL Aqr, 24", 352deg, 1966). SB2 (P = 4.08322d).
FL    Aqr    BDS 11854 B (A = FK Aqr; B 24", 352deg, 1966).
FO    Aqr    Brightness variations reveal Porb (see Table) and
FO    Aqr    Pspin = 0.014519d (the spin period varies).
FR    Aqr    VB A (B 16.68m V, white dwarf, 14", 311deg, 1946).
FS    Aqr    Min II = 13.2.
FU    Aqr    Type EW with twice longer period is also possible.
FV    Aqr    [Fe/H] = -2.8.
FW    Aqr    Min II = 13.15.
FX    Aqr    Blazhko effect?
FZ    Aqr    Min II = 14.7.
GH    Aqr    Min II = 13.1.
GI    Aqr    Min II = 14.2.
GK    Aqr    Min II = 12.8. P varies, current elements are given.
GM    Aqr    Min II = 14.3.
GN    Aqr    Min II = 12.10.
GR    Aqr    P = 0.675601d is also possible.
GS    Aqr    Min II = 13.5. According to [68018], P = 0.4604185d.
GV    Aqr    According to [N0002], P = 0.20259d.
HH    Aqr    Blazhko effect, P(Bl) = 68.7d ?
HI    Aqr    VB (a = 0.077", Porb = 19.25 yr). SB2 (P = 3.429616d).
HK    Aqr    Flare amplitude up to 0.6m U.
HL    Aqr    Rapid small-amplitude oscillations: P = 39.2s.
HM    Aqr    Very unusual, the depth of minima varies strongly.
HS    Aqr    Min II = 9.23.
HV    Aqr    Min II = 10.15. The X-ray source 1RXS J212125.1-030936. VB A (B 5", 321deg,
HV    Aqr    1992). The light curve shape varies.
HZ    Aqr    Porb = 3.7569d.
IO    Aqr    Min II = 9.17.
KQ    Aqr    The X-ray source 1RXS J221038.4-240120.
KV    Aqr    VB AB (A 7.24m; B 8.23m, 7", 158deg, 1991). One deep fading
KV    Aqr    on a brightening trend.
KX    Aqr    Min II = 8.47.
LL    Aqr    Min II = 9.59. The phase of MinII is 0.32.
LY    Aqr    A binary millisecond pulsar with radio eclipses.
LZ    Aqr    Orbital-period modulation during the bright stage:
LZ    Aqr    Min = 2451022.782 + 0.24820d * E [N0131].
MO    Aqr    Min II = 10.26.
MU    Aqr    Min II = 11.62.
NN    Aqr    Min II = 14.1.
NO    Aqr    Min II = 14.70.
NP    Aqr    Min II = 7.64.
NQ    Aqr    Min II = 12.8.
NW    Aqr    Min II = 14.1.
OV    Aqr    A twice longer period is not excluded.
QT    Aqr    Porb = 0.074665d.
QU    Aqr    Porb = 0.08330d.
QV    Aqr    VB A (B 19.1mg, 4", 228deg, 2001). Porb = 0.07196d.
QW    Aqr    The first-overtone period is tabulated. P0 = 0.47722d, A1/A0 = 1.3.
QZ    Aqr    Superhumps: P = 0.064593d? [233].
V0349 Aqr    Pspin is tabulated. Porb = 0.1344d.
V0354 Aqr    Blazhko effect, P = 181.20d.
V0357 Aqr    P varies. dP/dt = -0.37 x 10^(-5) d/yr.
V0358 Aqr    Epoch of minimum is tabulated. High states: 15.7 - 16.8m; low states: 16.5 - 17.5m.
V0360 Aqr    Blazhko effect, P = 54.52d.
V0362 Aqr    Light elements for eclipses are tabulated. DSCTC: P = 0.038213d, Delta m = 0.03m.
R     Aql    Period decreases, current elements are given. OH, H2O, SiO maser.
U     Aql    SB, Porb = 1856.4d. VB A (B 11.7m, 2", 224deg, 2009).
V     Aql    Biperiodic, P0 is tabulated, P1 = 215d.
W     Aql    SiO maser.
Y     Aql    Speckle binary (0.3").
Z     Aql    H2O maser.
RR    Aql    OH, H2O, SiO maser.
RS    Aql    OH, H2O, SiO maser.
SV    Aql    OH, H2O maser.
SY    Aql    OH, H2O, SiO maser.
SZ    Aql    P varies, current elements are tabulated.
TU    Aql    VB A (B 10.9m, 9", 356deg, 2000).
TW    Aql    OH maser.
UU    Aql    Porb = 0.163532d.
UX    Aql    VB A (B 4", 123deg).
VX    Aql    Double maxima.
XZ    Aql    P varies, current elements are tabulated.
YY    Aql    IR excess.
YZ    Aql    d = 0.03P. P varies, current elements are tabulated.
AA    Aql    [Fe/H] = -0.58.
AK    Aql    VB A (B 12.4m, 17", 86deg, 1999).
BC    Aql    [Fe/H] = 0.1.
BF    Aql    Multiple.
CD    Aql    VB, the SW component varies. Combined magnitudes are tabulated.
CI    Aql    The first outburst was detected in 1917. Eclipsing variations in quiescence: 15.3-16.2-15.7mV, Min = 2448412.167 + 0.618355d x E, D = 0.20:P [N0252].
CL    Aql    Multiple.
CR    Aql    Blazhko effect?
CS    Aql    VB A (B p).
DM    Aql    VB A (B 13.2m, 14", 178deg; C 14.0m, 8", 12deg, 1996).
DO    Aql    Eclipses: variable amplitude of the orbital variations, up to 0.8m. Min = 2448832.4408 + 0.167762d x E [N0255].
EU    Aql    H2O, SiO maser.
EV    Aql    P varies, current elements are tabulated. [A/H] = -0.3.
EW    Aql    VB A (A 12.2mV; B 12.4mV, 16", 188deg, 2000).
EX    Aql    Double wave, RV Tauri-like.
FF    Aql    VB A (B 10.1m, 7", 144deg, 2002; Aa, Ab 0.2", 157deg, 1990). SB1 (P = 1433d). P varies, quadratic term +84d x 10^(-10) x E^2.
FG    Aql    In the dark nebula B130.
FH    Aql    In the dark nebula B130.
FK    Aql    P varies, current elements are tabulated.
FN    Aql    P varies, current elements are tabulated.
FO    Aql    Porb = 0.217d.
FY    Aql    VB A (B 14.5:mV, 5", 219deg, 2000; B is a blend).
FZ    Aql    VB A (B 11.5m, F2V, 15", 163deg, 1999). The combined brightness in the ASAS photometry varies between 10.02m and 10.12mV.
GK    Aql    VB A (A 13m:V; B 13.1mV, 24", 3deg, 1999). Available deep surveys do not show a large amplitude.
GU    Aql    d = 0.02P.
GY    Aql    OH, SiO maser.
GZ    Aql    VB?
HI    Aql    VB A (B 14.1m, 26", 332deg, 2000).
II    Aql    VB A (B 15.4m, 10", 39deg, 1996; C 15.5m, 13", 235deg, 1996).
IM    Aql    P varies, the tabulated elements are valid between JD 2432772 and 2439000.
IQ    Aql    VB A (B 13.8m, 23", 168deg, 2000).
KL    Aql    [A/H] = 0.6.
KM    Aql    Blazhko effect, P = 192.20d.
KO    Aql    P varies, current elements are tabulated.
KX    Aql    Porb = 0.06035d.
LS    Aql    A wave with a cycle of 50-60d and an amplitude about 0.2-0.3m is superposed.
LT    Aql    Several companions at distances between 16" and 34".
MQ    Aql    VB A (B 8", 109deg, 1998).
MV    Aql    VB B (A 7.1mJ, B 10.0mJ; AB 6", 77deg, 2000).
OO    Aql    P varies, current elements are tabulated.
OP    Aql    P varies, current elements are tabulated.
OS    Aql    VB A (7.1mJ; B 11.3mJ, 8.5", 171deg, 1999).
PP    Aql    [A/H] = 0.0. P varies, current elements are tabulated.
PQ    Aql    Porb = 0.24675d.
QS    Aql    VB AB (6.69m, 6.75m, 0.2", 311deg, 2010).
QY    Aql    P varies, current elements are tabulated.
V0337 Aql    P varies?
V0341 Aql    [Fe/H] = -1.22.
V0342 Aql    VB B (A 8.3mV, B 8.7mV; AB 20", 14deg, 1999). P varies, current elements are tabulated.
V0343 Aql    P varies, current elements are tabulated.
V0346 Aql    VB A (B 11.4m, 3", 244deg, 2012); the magnitude in the table are for combined brightness. P varies, current elements are tabulated.
V0360 Aql    VB A (B 15.3mpg, 3", 215deg).
V0368 Aql    Eclipses: Min = 2449189.5230 + 0.69050942d x E, amplitude about 0.25mR [N0263].
V0379 Aql    VB A (A 9.1mJ; B 13.6mJ, 6", 1998). Combined magnitudes are tabulated.
V0387 Aql    VB A (B 15.0mV, 8", 332deg, 1999; also other components).
V0409 Aql    Spectral type A2-A3 in a different publication.
V0413 Aql    A very unusual light curve, with a large (up to 0.5mV) scatter outside of minima. IR excess?
V0417 Aql    P varies, current elements are tabulated.
V0418 Aql    P varies? Current elements are tabulated.
V0419 Aql    Superposed shorter (80d - 100d) waves with an amplitude about 0.3m.
V0434 Aql    Several companions within 40".
V0435 Aql    Several companions within 25".
V0441 Aql    Often exhibits double maxima.
V0455 Aql    OH, H2O maser.
V0459 Aql    VB A (B 15m, 8", 131deg).
V0461 Aql    VB A (B 14.2m, 8", 286deg, 1990).
V0466 Aql    VB A (B 11.0m, 22", 19deg, 2000).
V0470 Aql    H2O maser.
V0483 Aql    In the region of the open cluster NGC 6709. A cycle about 927d is possible.
V0484 Aql    VB B (A 11.0mV, B 12.2mV; AB 26", 84deg, 1999).
V0486 Aql    VB A (B 15.0mV, 9", 276deg).
V0497 Aql    VB A (B 15.2mV, 10", 26deg, 1993).
V0500 Aql    Eclipses: P = 0.1452d, depth about 0.4m [N0264].
V0502 Aql    VB A (B 5", 335deg); combined magnitudes are tabulated.
V0522 Aql    VB A (A 8.9mJ, B 12.7mJ; AB 5", 249deg, 1998); combined magnitudes are tabulated.
V0526 Aql    P varies? Current elements are tabulated.
V0528 Aql    VB A (B 16.3m, 10", 74deg, 1951).
V0530 Aql    VB A (B 13.0mR, 24", 18deg, 1999; C 13.2mR, 16", 336deg).
V0535 Aql    VB A (B 15.6m, 9", 279deg, 1999).
V0536 Aql    Speckle-interferometric binary (0.5", 17deg).
V0539 Aql    VB A (B 15.2mpg, 7", 235deg).
V0556 Aql    VB A (B 7", 270deg).
V0557 Aql    P varies, current elements are tabulated.
V0561 Aql    VB A (12.5:mV; B 13.6mV, 22", 205deg, 1999; C 14.1mV, 20", 169deg, 1999).
V0572 Aql    P varies, current elements are tabulated. [Fe/H] = 0.0.
V0602 Aql    P varies, current elements are tabulated.
V0603 Aql    Porb = 0.13815d, reflected in the X-ray flux and polarization. Variations at minimum brightness: 11.62-12.15mV, Positive (0.144-0.145d) and negative (about 0.135d) superhumps, quasi-peri
V0605 Aql    VB A (B 15.6m, in 8" sf). A maximum was observed in 1919, with secondary brightenings. Faint after 1923. In the center of the planetary nebula A58. Probably an event of the final helium
V0609 Aql    VB A (B 5", 90deg, 1998). Combined magnitudes are presented. P varies? Currents elements are tabulated.
V0635 Aql    VB A (B 13.8m, 13", 187deg, 1999). The tabulated magnitudes are influenced with the companion. OH maser.
V0641 Aql    VB B (A 13.6m; AB 14", 303deg, 2000).
V0654 Aql    VB B (A 12.8m; AB 20", 305deg, 2000). The tabulated magnitudes are probably influenced with the companion.
V0666 Aql    VB A (B 5", 356deg, 1997). Combined magnitudes are tabulated.
V0672 Aql    Blazhko effect?
V0676 Aql    VB A (A 13.8mV; B 14.2mV, 12", 51deg, 2000).
V0694 Aql    VB A? (B 1").
V0703 Aql    VB A (7.54mK; B 8.82mK, 23", 90deg).
V0724 Aql    P varies? Current elements are tabulated.
V0725 Aql    VB A (B 12.7m; AB 13", 10deg, 1991).
V0734 Aql    VB A (B 16.3m, 7", 114deg, 1997).
V0755 Aql    The light elements Min = 2429195.290 + 1.01598d x E are not excluded.
V0761 Aql    P varies? Current elements are tabulated.
V0762 Aql    The period 2.1d/N [00387] cannot be confirmed with more recent epochs of minima.
V0766 Aql    [Fe/H] = -1.98.
V0778 Aql    VB A (B 13.2m, 20", 18deg, 2000; C 13.4m, 13", 78deg, 2000).
V0780 Aql    OH maser.
V0782 Aql    VB A (B 15.9mV, 6", 322deg, 2000).
V0793 Aql    [Fe/H] = -1.53.
V0801 Aql    VB A (B 14.0m, 14", 240deg, 1999).
V0803 Aql    P varies, current elements are tabulated.
V0812 Aql    VB A (B 14.4mV, 11", 122deg, 1999; C 6", 226deg).
V0814 Aql    VB A (13.8mR; B 15.8mR, 8", 236deg, 1999).
V0819 Aql    VB B (A 13.3mV; B 14.1mV, 11", 235deg, 1999).
V0822 Aql    VB A (B 9.6m, 1", 70deg, 1991; C 10.5m, 297deg, 2003).
V0825 Aql    VB A (12.4mV; B 13.3mV, 26", 236deg, 1999; C 13.4mV, 18", 213deg, 1999).
V0829 Aql    Multiperiodic.
V0845 Aql    VB A (B 13.2m, 29", 28deg, 2000).
V0846 Aql    Modern photometric surveys do not confirm the tabulated variability data.
V0866 Aql    VB A (B 5"s).
V0871 Aql    MinII - MinI = 0.55P.
V0877 Aql    VB A (B 16.5mpg, 6", 49deg, 1999; C 17.2mR, 7", 155deg, 1999).
V0878 Aql    VB A (11.6mV; B 12.0mV, 21", 180deg, 1999).
V0888 Aql    VB C (A 12.4mV, B 13.0mV; AC 18", 307deg, 1999; BC 23", 111deg, 1999). In the region of the open cluster NGC 6738.
V0889 Aql    MinII - MinI = 0.36P. P varies, current elements are tabulated. Light-time effect, apsidal motion?
V0895 Aql    [Fe/H] = -0.54.
V0909 Aql    VB A (14.4mR; B 15.7mR, 8", 171deg, 1998; C 16.0mR, 19", 100deg, 1998).
V0912 Aql    VB A (B 13.6m, 12", 309deg, 1999).
V0913 Aql    The tabulated period corrects a misprint in [08717].
V0917 Aql    d = 0.03P.
V0923 Aql    Periodic variations with P = 0.8518d were reported in [03178]. SB, P = 214.756d.
V0926 Aql    P varies? Current elements are tabulated.
V0927 Aql    VB B (A 14.2mV, B 14.9mV; AB 7", 328deg, 1999).
V0936 Aql    P varies, current elements are tabulated. VB B (A 13.3mV, B 13.6mV; AB 11", 35deg, 2000).
V0958 Aql    VB A (A 15.4mV; B 15.7mV, 8", 57deg, 1999; C 16.1mV, 12", 313deg, 1999).
V0962 Aql    P varies, current elements are tabulated.
V0965 Aql    VB A (B 14.7mV, 11", 118deg, 1998).
V0968 Aql    Multiple.
V0971 Aql    [Fe/H] = -0.3.
V0991 Aql    Multiple.
V0999 Aql    Observations from [07806] contradict the tabulated elements.
V1012 Aql    P2 = 83.7d, P3 = 1146d.
V1019 Aql    VB A (A 12.7mV; B 16.7mV, 16", 196deg, 1997; also fainter companions).
V1046 Aql    P varies?
V1058 Aql    VB A (A 12.5mJ; B 13.9mJ, 11", 225deg, 1998).
V1062 Aql    OH, H2O maser.
V1069 Aql    VB (4").
V1070 Aql    VB B (A 14.0mV, B 14.1mV; AB 12", 160deg, 2000).
V1076 Aql    VB B (A 14m; AB 12", 284deg, 1998).
V1086 Aql    VB A (B 7", 291deg, 2000). Combined magnitudes are tabulated.
V1096 Aql    P varies, current elements are tabulated.
V1101 Aql    Porb = 0.1442d.
V1102 Aql    P = 0.594045d is also possible.
V1112 Aql    MinII - MinI = 0.30P?
V1132 Aql    VB B (A 14.1V; AB 5", 228deg, 2000).
V1140 Aql    P varies?
V1147 Aql    VB B (A 12.6m; AB 24", 259deg, 1998).
V1154 Aql    MinII - MinI = 0.70P.
V1166 Aql    Type UG is also possible.
V1173 Aql    VB A (B 17.6m, 13", 241deg, 2000).
V1199 Aql    Not red.
V1204 Aql    VB A (B p).
V1208 Aql    Multiperiodic.
V1215 Aql    The tabulated period can be a multiple of the true one.
V1248 Aql    OH, H2O maser.
V1251 Aql    Another solution from different data: EB:, 13.0m - 13.7mV, MinII 13.5mV, Min = 2451443 + 0.49942d x E.
V1269 Aql    VB A (B 7", 43deg, 1999). Combined magnitudes are tabulated.
V1285 Aql    SB2, Porb = 10.3191d.
V1286 Aql    Rapid oscillations: P = 11.6 minutes, multiperiodic, amplitude about 0.001mB [N0287].
V1293 Aql    Long-term variations: P = 270:d.
V1297 Aql    d = 0.05P.
V1298 Aql    A flare was detected spectroscopically [06835]. A common-proper-motion companion of BD+04 4048.
V1300 Aql    OH, SiO maser.
V1302 Aql    OH, SiO maser. Was gradually brightening in 1925 - 1970. Becomes gradually hotter. A protoplanetary object?
V1309 Aql    P = 6.97d/N.
V1319 Aql    H2O maser.
V1323 Aql    Several companions.
V1325 Aql    VB A (B 4" sf).
V1333 Aql    Aql X-1. VB B (A 19.4m; B 0.5" p). Outbursts once in several months.
V1338 Aql    VB B (A 15.8mR; B 16.0mR, 6", 84deg, 1999).
V1339 Aql    SB?, P = 1.27219d. Speckle-interferometry binary, rho = 0.057".
V1340 Aql    d = 0.06P:. Intrinsic brightness variations outside eclipses are possible.
V1342 Aql    P varies, current elements are tabulated.
V1343 Aql    SS 433. B - V = +2.0m. Associated with the SNR W 50. The light elements
V1343 Aql    for eclipses are tabulated. Eclipses: the depth of MinI varies
V1343 Aql    between 0.2 and 0.9m; that of MinII, between 0 and 0.4m.
V1343 Aql    The mean light varies between 14.0m and 14.6m with the period
V1343 Aql    162.15d, which varies; this period is usually interpreted as
V1343 Aql    precession of the accretion disk. Also noted is the period
V1343 Aql    6.2877d, interpreted as nutation. Different kinds of activity
V1343 Aql    and irregularity are present in the light curves. Three systems
V1343 Aql    of H, HeI, HeII emission lines are observed in the spectrum: the
V1343 Aql    "stationary" one, featuring radial velocity variations between 150
V1343 Aql    and 300 km/s with the orbital period, and two "relativistic" ones, with radial velocity
V1343 Aql    variations, opposite in phase, between -35000 and +50000 km/s.
V1343 Aql    The "relativistic" systems correspond to two jets consisting of
V1343 Aql    high-density condensations of matter emerging from the system at
V1343 Aql    a relativistic velocity (0.27 c). The system is generally considered
V1343 Aql    a prototype microquasar, but its properties remain extreme for the
V1343 Aql    whole class of such objects.
V1352 Aql    VB A (B 14.6m, Sp M3, 6", 172deg, 1999). A chain of Herbig - Haro objects near the variable.
V1355 Aql    P varies?
V1360 Aql    OH, SiO maser.
V1361 Aql    OH, SiO, H2O maser.
V1362 Aql    OH, SiO, H2O maser.
V1363 Aql    OH maser.
V1364 Aql    OH, SiO, H2O maser.
V1365 Aql    OH, SiO, H2O maser.
V1366 Aql    OH, SiO, H2O maser.
V1367 Aql    OH, SiO maser.
V1368 Aql    OH, SiO, H2O maser.
V1369 Aql    OH, SiO maser.
V1376 Aql    VB (9", 356deg, 2000). The light elements need verification.
V1379 Aql    The period of RS variations is tabulated. Eclipses:
V1379 Aql    Min = 2449656.4804 + 20.66118d x E, D = 0.07P, d = 0.06P, depth 0.17mU.
V1401 Aql    P2 = 11.8d. [Fe/H] = -1.1.
V1402 Aql    Multiple. Probably multiperiodic.
V1405 Aql    The tabulated light elements are for eclipse-like fadinds, there amplitude being about 0.4m - 0.5m.
V1406 Aql    VB B (A 7.03mV, B 11.3mV; AB 10", 180deg, 2012).
V1408 Aql    The tabulated elements are for the maximum of small-scale periodic variations.
V1413 Aql    d = 0.05P. The depth of eclipses outside outburst peaks is about 2m.
V1415 Aql    OH, SiO, H2O maser.
V1416 Aql    OH, SiO, H2O maser.
V1427 Aql    Possibly a protoplanetary object.
V1433 Aql    OH, H2O maser.
V1436 Aql    VB A (9.4mV; B 12.3mV, 4", 33deg, 2001). Possibly spurious variability.
V1440 Aql    VB A (8.6mV; B 9.9mV, 22", 198deg, 2013).
V1452 Aql    P = 2.5930d is also possible.
V1461 Aql    VB AB (9.3m, 10.5m, 2.5", 306deg, 2002).
V1462 Aql    VB A (8.3mV; B 11.5mV, 13", 88deg, 2000).
V1466 Aql    VB A (6.5mV; B 10.3mV, 14", 310deg, 2012).
V1470 Aql    VB AB (8.2m, 9.2m, 2", 286deg, 2011). Probably the fainter component varies.
V1472 Aql    VB AB (6.6mV, 11.0mV; 3", 120deg, 2008). SB, Porb = 198.716d.
V1473 Aql    Multiperiodic, P2 = 2.04036d, P3 = 3.41274d.
V1477 Aql    VB AB (9.73mV, 12.56mV, 1", 2deg, 1991). Another companion: 9.2mR, 20", 112deg, 1998. Possibly spurious variability.
V1479 Aql    The spectral type presented in the Hipparcos catalog (K7) contradicts the star's color indices. Possibly spurious variability.
V1488 Aql    Erroneously called GM Aql in several publications by V.P. Tsesevich.
V1494 Aql    VB A (B 18.1m, 1"). Eclipses: Min = 2452462.4966 + 0.1346141d x E, depth 0.25m, D = 0.20P [N0308].
V1532 Aql    Several companions.
V1538 Aql    Possible RRC periods: 0.3661945d, 0.2678428d.
V1546 Aql    VB B (A 10.3mV; B 11.52mJ, 11.22mK, 16", 299deg, 2000).
V1575 Aql    In the region of the globular cluster NGC 6749.
V1576 Aql    In the region of the globular cluster NGC 6749.
V1648 Aql    Brightening over 10 years, probably due to dissipating dust envelope, plus quasi-periodic variations. [Fe/H] = -1.1.
V1656 Aql    The tabulated ephemeris is for eclipses. P varies, quadratic term +1.14 x 10^(-6)d x E^2.
V1656 Aql    Instead, period jumps are not excluded. Occasional brightness humps: P = 8.628d.
V1665 Aql    MinII - MinI = 0.40P. Slight apsidal motion.
V1706 Aql    Epoch of minimum brightness is tabulated.
V1707 Aql    VB A (B 13.9m, 18", 166deg, 1999).
V1710 Aql    Epoch of maximum is tabulated. Continuous periodic brightness variations.
V1719 Aql    A twice longer period is not excluded.
V1737 Aql    VB A (B 12.2mV, 7", 130deg, 2000).
V1742 Aql    VB A (B 16.5m, 2" sp).
V1743 Aql    The elements tabulated are for EB variations. EA: amplitude 0.14m, Min = 2450646.6692 + 1.1920d x E, D = 0.14P.
V1752 Aql    P2 = 0.3586d.
V1760 Aql    P2 = 0.8381d.
V1801 Aql    An asymptotic-giant-branch star. SB, Porb = 119.5d, e = 0.37. Porb is not detected in photometry.
V1811 Aql    A twice shorter period is not excluded.
V1815 Aql    A magnetic white dwarf, varies presumably due to starspots and axial rotation.
V1820 Aql    O'Connell effect.
alf   Aql    Multiperiodic.
eta   Aql    The presence of an unresolved A0V companion is suspected. P varies, current elements are tabulated.
R     Ara    Min II 6.2. The light curve shape outside eclipses varies.
R     Ara    VB A (B 8.2m, 4", 123deg, 1933).
S     Ara    [Fe/H] = -0.71. P var. Max = 2420047.2382 + 0.451888176d*E -
S     Ara    1.36d*10**(-10)*E**2 (2414000 - 2441200) [03126]. For current
S     Ara    elements after 2441000, see Table.
T     Ara    VB A (B 11.0m, 34", 60deg).
RW    Ara    d = 0.02P, Min II = 8.91. Changes of the shape of the light curve
RW    Ara    due to gaseous streams or to a hot spot are possible.
SY    Ara    Min II = 10.60.
SZ    Ara    P var [00005].
TV    Ara    In the region of the open cluster NGC 6208.
TX    Ara    VB A (B 16.5m 5" sf). A twice shorter period is possible.
UW    Ara    Min II = 9.53.
XX    Ara    Min II = 14.1.
AA    Ara    Min II = 13.3.
AD    Ara    [A/H] = -0.4.
AF    Ara    Min II = 13.8.
AW    Ara    Before JD 2417300, Max = 2412600 + 186d*E.
BF    Ara    The superoutburst cycle is given.
CC    Ara    VB A (B 14.9m 7" sp).
CL    Ara    Min II = 13.6.
CT    Ara    Between JD 2420400 and 2425000, Max = 2413080 + 215d:*E.
CY    Ara    Min II = 12.6.
DU    Ara    P var.
DZ    Ara    VB A (B 12.9m 12" np).
EH    Ara    VB A (B 14.7m 12" nf).
EK    Ara    VB A (B 15m pg 5" s).
ER    Ara    Min II = 14.2.
FR    Ara    Min II = 12.0.
FS    Ara    VB A (B 15.1m V 7" nf).
FT    Ara    VB A (B 15.4m 7" nf).
FU    Ara    Min II = 10.60.
GI    Ara    VB A (B 10" sp). It is not quite clear which star varies.
GK    Ara    The coordinates in [00051] and the chart in [00034] are
GK    Ara    believed to be wrong.
GM    Ara    Min II = 13.1.
IN    Ara    [Fe/H] = -1.75.
IT    Ara    Min II = 12.2.
IW    Ara    VB A (B 15.9m 9" sp).
KO    Ara    Min II = 13.4.
KP    Ara    VB A (B 14.8m 7" p).
KU    Ara    Min II = 13.1.
KY    Ara    Only one sharp Max (JD2428715 - 721) was observed [00055].
KY    Ara    Possibly a Nova.
KZ    Ara    VB A (B 13.5m 13" p).
LP    Ara    Min II = 10.4.
LR    Ara    Min II = 11.01.
LU    Ara    Min II = 10.4.
LW    Ara    As of May 2006, erroneously called LX Ara in [00002].
MM    Ara    Min II = 11.85.
MQ    Ara    VB A (B = NSV 09784 25" sp).
MR    Ara    [Fe/H] = -1.0.
MS    Ara    [Fe/H] = -1.48.
MT    Ara    VB A (B 13.5m 26" sf).
MV    Ara    VB A (B 17.6m 7" nf), a star 13.5m 18" n.
MX    Ara    VB A (B 15.5m 14" sf).
NO    Ara    Min II = 13.0 V.
NU    Ara    VB B (A 16.4m 8" sp).
OY    Ara    Eclipsing variations [00010]: amplitude 1.9m (wide B+V filter),
OY    Ara    Min = 2449862.8220 + 0.155466d*E.
QR    Ara    Marked in the chart for BV 1443. ASAS-3 data do not show
QR    Ara    noticeable variations.
QX    Ara    Erroneously called V675 Ara in [00002].
V0336 Ara    Min II = 12.3.
V0340 Ara    [A/H] = 0.6.
V0341 Ara    X-ray source 1RXS J165743.7-631237. V-Ic between 0.08m and
V0341 Ara    0.20m [00012]. The periods 11.95d [00111], 10.919d [00075],
V0341 Ara    14.11045d [00012] satisfy observations only during some
V0341 Ara    intervals of time.
V0342 Ara    P >= 140d.
V0345 Ara    P >= 180d.
V0349 Ara    Min II = 8.93.
V0355 Ara    P > 220d.
V0356 Ara    P > 170d. VB B (A 12.65m B, 22" nf).
V0360 Ara    Min II = 13.8. Min II - Min I = 0.35P.
V0361 Ara    Min II = 13.6.
V0362 Ara    Min II = 15.6.
V0383 Ara    VB A (B 16.5m 8" nf).
V0419 Ara    Not red [00000].
V0421 Ara    Min II = 15.1.
V0422 Ara    According to [00054] and [00053], UG. The spectral type suggests
V0422 Ara    another type [00013].
V0433 Ara    Eclipses: Min = 2453065.5502 + 0.19573d*E [00014]. According to
V0433 Ara    [00014], the outside-eclipse brightness varies between 16.8m
V0433 Ara    and 18.4m V, suggesting a type like NL+EA or UGZ+EA. The
V0433 Ara    faintest magnitude observed in an eclipse was about 19.6m V.
V0440 Ara    Min II = 14.5.
V0444 Ara    Min II = 14.2.
V0447 Ara    Another possible solution of the data from [00002]:
V0447 Ara    Min = 2451936.878 + 18.146d*E [00015].
V0454 Ara    Min II = 13.6.
V0461 Ara    Identified with a bright IR object in the 2MASS catalogue.
V0480 Ara    Min II = 15.5.
V0482 Ara    Min II = 13.5.
V0485 Ara    Min II = 14.8.
V0489 Ara    Min II = 12.4.
V0491 Ara    Min II = 12.8.
V0492 Ara    Min II = 14.5.
V0497 Ara    Min II = 13.4.
V0501 Ara    Min II = 13.8.
V0520 Ara    No objects with Mira-like colors in the field [00000].
V0528 Ara    Not an RR Lyrae star according to [00006], where no period
V0528 Ara    could be found between 0.25d and 2.0d.
V0529 Ara    Min II = 13.1.
V0531 Ara    Min II = 11.25.
V0532 Ara    Min II = 11.5.
V0535 Ara    Min II = 7.71.
V0536 Ara    Min II = 11.8.
V0537 Ara    Min II = 8.91.
V0539 Ara    Min II = 6.16. VB A (B 9.22m, 12", 269deg). DII = 0.13P. Apsidal motion.
V0539 Ara    Tabulated are: the epoch of MinI based on observations in [00075]
V0539 Ara    and the siderial period from [00017]. In 1982 - 1994,
V0539 Ara    MinI = 2445056.777 + 3.169112d*E,
V0539 Ara    MinII = 2445067.825 + 3.169076d*E, U = 150 years. The fainter
V0539 Ara    component of the eclipsing pair pulsates, the detected periods
V0539 Ara    are 1.36d, 1.78d, 1.08d [00017].
V0544 Ara    Min II = 13.8. VB A (B 14.5m pg, 17" sp).
V0562 Ara    Min II = 13.9.
V0577 Ara    The chart in [00059] leads to a much brighter star than the
V0577 Ara    magnitudes in [00059]; for this brighter star, the data in
V0577 Ara    [00002] permit to suspect type EA, Max 13.1m V, MinI 13.6m V,
V0577 Ara    MinII 13.3:m V, MinI = 2453090.826 + 0.6880d*E, with a large
V0577 Ara    light-curve scatter [00000].
V0583 Ara    The chart in [00059] leads to a much brighter star than the
V0583 Ara    magnitudes in [00059].
V0613 Ara    VB B (A 12" np).
V0616 Ara    Min II = 8.47.
V0617 Ara    VB B (A 13.1m Bj, 12" nf). Combined magnitudes of the pair are
V0617 Ara    given.
V0624 Ara    MaxII 11.9 at the phase 0.4.
V0639 Ara    V1 (NGC 6397). Cluster non-member.
V0650 Ara    Individual cycles have amplitudes about 0.7m, the mean
V0650 Ara    brightness level varies.
V0651 Ara    Min II = 15.3.
V0653 Ara    Min II = 13.0.
V0656 Ara    EW type is not excluded.
V0658 Ara    Min II = 16.0. The suggested type is in contradiction with
V0658 Ara    the star's red color [00000].
V0659 Ara    Min II = 14.4.
V0668 Ara    Min II = 13.8.
V0687 Ara    Type RRC is possible.
V0700 Ara    Min II = 15.7.
V0702 Ara    Min II = 14.0.
V0705 Ara    Min II = 14.4.
V0710 Ara    Individual cycles have amplitudes from 0.5m to 1m, secondary
V0710 Ara    cycle about 750d.
V0722 Ara    Min II = 10.09.
V0728 Ara    Min II = 13.5.
V0729 Ara    Type RV with a twice longer period is possible.
V0740 Ara    Min II = 13.5.
V0744 Ara    Not red.
V0755 Ara    The chart in [00112] (BV 1310) shows a different variable star.
V0781 Ara    Min II = 14.8.
V0783 Ara    Min II = 13.9.
V0789 Ara    Min II = 14.8.
V0790 Ara    Min II = 14.8.
V0791 Ara    Min II = 13.1.
V0792 Ara    Min II = 15.2.
V0793 Ara    Not red.
V0801 Ara    MXB 1636-53. Description of the spectrum [00113].
V0801 Ara    Modulation with Porb = 0.15804738d [00020], amplitudes up to
V0801 Ara    0.6m V.
V0808 Ara    Type EW is possible.
V0816 Ara    Type RR: was suggested in [00053], but the star is red.
V0820 Ara    Epoch of Min is given. Strong magnetic field. Either an
V0820 Ara    eclipsing binary or a white-dwarf oblique rotator.
V0821 Ara    4U 1658-48. Complex behavior. Three X-ray states: off, hard-low,
V0821 Ara    high-soft, poorly correlated with optical variations. The latter
V0821 Ara    consist of flickering, possible low-amplitude quasi-periodic
V0821 Ara    variations, and large-amplitude changes. Porb near 0.7d is
V0821 Ara    suspected.
V0825 Ara    V2 (NGC 6397), cluster non-member.
V0826 Ara    V3 (NGC 6397), cluster non-member.
V0827 Ara    V4 (NGC 6397) according to the numbering system from [67025] (differs from the numbering system in [N0025]). Probably cluster non-member.
V0829 Ara    Type SRB is possible [00114]. According to [00075], ELL,
V0829 Ara    6.06m - 6.14m Hp, Min = 2448504.951 + 7.5010d*E; these type and
V0829 Ara    period seem improbable for the spectral type.
V0832 Ara    Porb = 5200d.
V0834 Ara    Oscillations: P = 12 minutes.
V0835 Ara    Oscillations: P = 10.75 minutes.
V0837 Ara    Associated with a nebula.
V0839 Ara    Associated with a nebula.
V0851 Ara    Min II = 6.97.
V0852 Ara    Min II = 7.94.
V0867 Ara    Min II = 7.57.
V0870 Ara    Min II = 9.40.
V0878 Ara    Min II = 8.21.
V0881 Ara    Min II = 10.57.
V0883 Ara    MinII - MinI = 0.44P.
V0898 Ara    Multiperiodic.
V0909 Ara    Called "BH Ara?" in [80474]; the suggested identification is wrong.
R     Ari    H2O, OH maser.
T     Ari    H2O, SiO maser. P varies strongly, current elements are given.
U     Ari    SiO maser.
W     Ari    A "missing BD star", no certain identification.
X     Ari    P varies, current elements are given. [Fe/H] = -2.50.
RS    Ari    Min II = 11.0.
RU    Ari    OH, H2O maser.
RV    Ari    Double-mode. P0 is given in the Table, P1 = 0.0719469d. Both
RV    Ari    periods vary.
RW    Ari    [Fe/H] = -1.16.
RX    Ari    d = 0.02P, Min II = 9.5. P varies, current elements are given.
RY    Ari    H2O maser.
SS    Ari    Min II = 10.5. P varies, current elements are given.
SU    Ari    A "missing BD star", identification uncertain.
SZ    Ari    P varies, current elements are given.
TT    Ari    Porb = 0.13755d. Usually near maximum brightness, occasional
TT    Ari    deep fadings. Numerous photometric periods were reported.
TT    Ari    According to [N0138], the star experiences alternating
TT    Ari    "negative superhump" (P = 0.13270 - 0.1398d) and "positive
TT    Ari    superhump" (P = 0.14840 - 0.14926d) intervals, with amplitudes
TT    Ari    of several tenths of a magnitude. Quasiperiodic oscilations,
TT    Ari    flickering.
TU    Ari    P varies, current elements are given.
TX    Ari    P varies, current elements are given.
UU    Ari    Multiperiodic.
UV    Ari    Probably multiperiodic.
UX    Ari    VB (0.4", 61deg, 1990.8). SB2, Porb = 6.43791d. Photometric
UX    Ari    variations with a period close to Porb. Mean brightness varies.
VW    Ari    Multiperiodic.
VY    Ari    SB1, Porb = 13.20d.
WW    Ari    VB (3"). Probably both components vary.
WX    Ari    The elements are for eclipses. Flickering.
XZ    Ari    Min II = 14.0.
YY    Ari    H2O, OH maser.
YZ    Ari    OH maser.
AD    Ari    Min II = 7.4. According to [N0146], DSCTC pulsations with a period about
AD    Ari    0.06d can be also present.
AG    Ari    Min II = 8.3.
AL    Ari    Min II = 9.4.
AW    Ari    Min II = 14.3.
BF    Ari    Periodically variable brown dwarf.
BG    Ari    Porb = 0.082417d.
BI    Ari    Multiperiodic.
BM    Ari    Min II = 11.35.
BN    Ari    Min II = 10.98.
BO    Ari    Min II = 10.19.
BQ    Ari    Min II = 10.54. VB A (A 10.9m; B 11.5m, 14", 19deg, 2000). The tabulated magnitudes are possibly affected by the companion.
BS    Ari    VB (0".5, 104deg, 2001).
BU    Ari    VB (0".4, 52deg, 2001); VB A (B 4", 61deg, 2001; C = LkHA 263, 15", 23deg, 2001).
BV    Ari    VB (0".4, 234deg, 2001); VB C (A = LkHA 262; AC 15", 23deg, 2001).
BX    Ari    VB AB (1", 165deg, 2001).
CL    Ari    Min II = 10.00.
gam   Ari    VB A (B 4.65m, B9V, 8", 0deg).
tau 1 Ari    VB AB (B 8.4m V, 0.7", 246deg, 1968).
R     Aur    H2O, SiO maser. P varies, current elements are given.
T     Aur    Eclipses: Min = 2452283.261 + 0.20437826d * E. The minima from
T     Aur    0.10m to 0.28m deep in integrated light [03195].
U     Aur    OH, H2O, SiO maser.
Z     Aur    P varies, current elements are given.
RS    Aur    Biperiodic, the second period is 168d [N0039].
RT    Aur    P varies, current elements are given.
RU    Aur    OH, SiO maser.
RW    Aur    VB ABC (1.4", 255deg, 1994; B 13.6m, K5, suspected in flare
RW    Aur    activity; BC 0.12").
RX    Aur    P varies [N0147]. Elements for 1990s are given in the Table.
RX    Aur    [Fe/H] = -0.13.
RY    Aur    P varies, current elements are given.
RZ    Aur    P varies, current elements are given.
SS    Aur    Porb = 0.1828d. Intervals of abnormal photometric behavior
SS    Aur    (frequent low-amplitude outburts) occur sometimes.
ST    Aur    VB A (B 14m, 7" sp).
SU    Aur    OH maser.
SX    Aur    Min II =  8.87 .
SX    Aur    P varies, current elements are given.
SY    Aur    P varies, current elements are given.
SZ    Aur    SiO maser.
TT    Aur    Min II =  8.97 .
TW    Aur    The mean brightness varies with P = 1380d.
TZ    Aur    [Fe/H] = -0.79.
UU    Aur    Double-mode, also P = 235d.
UV    Aur    A symbiotic Mira. Very variable heights of maxima.
UV    Aur    [NeIII] and [OIII] emissions in the spectrum.
UV    Aur    VB A (B 10.96m, B9V, 3.4", 4deg).
UV    Aur    The B9V companion is apparently not hot enough to excite the
UV    Aur    nebula.
UW    Aur    Epoch of Min is given.
UY    Aur    OH maser. VB AB (B 12m?, M2, 0.9", 228deg, 1999).
VW    Aur    VB AB (9.0m, 11.8m V, 1.4", 332deg, 1976).
WW    Aur    Min II =  6.43 .
XX    Aur    Min II = 13.4  .
XX    Aur    P varies? Current elements are given.
YZ    Aur    SB.
ZZ    Aur    Min II = 11.04 .
AB    Aur    Rare deep fadings.
AE    Aur    The well-known "runaway star" from Ori OB1.
AH    Aur    The depth of MinII is 0.50m.
AM    Aur    Min II = 10.15 .
AM    Aur    P varies, current elements are given.
AO    Aur    P varies? Current elements are given.
AP    Aur    P varies, quadratic term 6.3398d*10^(-10)E^2. The depth of MinII
AP    Aur    is 0.51m.
AQ    Aur    SiO maser.
AR    Aur    Min II =  6.70 .
AR    Aur    P varies, current elements are given.
AR    Aur    Period variations are possibly periodic, with a period of
AR    Aur    25-27 years [N0158].
AW    Aur    SiO maser.
AZ    Aur    VB A (B 16.3m B, 4", 165deg, 1953).
BC    Aur    Min II = 11.7  .
BF    Aur    Min II =  9.48 .
BF    Aur    P varies, current elements are given.
CG    Aur    Min II = 12.05 .
CG    Aur    Apsidal motion? P(MinII)=1.8048647d.
CI    Aur    Min II = 12.45 .
CI    Aur    P varies, current elements are given.
CL    Aur    The depth of MinII is 0.32m Rc. P var. Quadratic term
CL    Aur    +2.52d*10^(-10)E^2. Third body, P = 21.7 years.
CO    Aur    The tabulated period is that of the first overtone; the second
CO    Aur    overtone period is 1.427781d.
CP    Aur    Min II = 13.3  .
CQ    Aur    Min II =  9.14:.
DN    Aur    [Fe/H] = -0.46. VB A (B 7", 46deg, 2000).
EI    Aur    Min II = 15.0  .
EM    Aur    Min II = 11.50 .
EM    Aur    P varies?
EO    Aur    Min II =  7.89 .
EP    Aur    P varies, current elements are given. The depth of MinII is
EP    Aur    0.22m.
EQ    Aur    Min II = 12.93 .
EQ    Aur    P varies, current elements are given.
ER    Aur    P varies, current elements are given.
EU    Aur    Min II = 12.9  .
EW    Aur    [Fe/H] = -0.6.
FF    Aur    [Fe/H] = -0.3.
FG    Aur    Min II = 12.1  .
FN    Aur    Min II = 12.2  .
FO    Aur    Min II = 14.0  .
FP    Aur    d =  0.08 P.
FR    Aur    Min II = 13.0  .
FS    Aur    Porb = 0.059479d.
FW    Aur    Min II = 12.5  .
FZ    Aur    A two times shorter period is also possible.
GI    Aur    Min II = 11.50:.
GX    Aur    Min II = 12.2  .
GX    Aur    P varies, current elements are given.
GY    Aur    Min II = 12.8  .
HL    Aur    Min II = 11.25 .
HN    Aur    The secondary period is about 1400d.
HP    Aur    Min II = 11.55 .
HS    Aur    Min II = 10.70 .
HU    Aur    Min II = 11.8  .
HW    Aur    Min II = 13.2  .
II    Aur    Min II = 15.0 :.
II    Aur    MinII 15.0:.
IM    Aur    Min II =  8.21 .
IS    Aur    VB A (B 15.4m, 18", 47deg, 1999). The tabulated range is for
IS    Aur    the combined magnitude of the pair.
IU    Aur    Min II =  8.74 .
IU    Aur    A well-documented light-time effect (P = 294.3d, the semi-amplitude
IU    Aur    of the O-C residuals is 0.0059d) because of a third body on
IU    Aur    an eccentric orbit. Precession causes changes of the brightness
IU    Aur    amplitude: the amplitude of the MinI was observed to vary between
IU    Aur    0.46m and 0.70m and that of MinII, between 0.37m and 0.55m. The
IU    Aur    depths of minima reached their maximum values about JD 2445800
IU    Aur    and began to decrease [N0176].
IY    Aur    Min II =  9.49 .
IZ    Aur    Min II = 13.4  .
KO    Aur    Min II = 10.45 .
KR    Aur    Porb = 0.1628d.
KU    Aur    Min II = 11.8  .
KU    Aur    P varies?
KW    Aur    VB A (B 9.0m, 10", 9deg, 2004; C 7.3m, F4V+DA1, Porb = 2.99d,
KW    Aur    14", 225deg, 1991). SB, Porb = 3.7886d. The pulsation period is
KW    Aur    tabulated. Other pulsation harmonics: 0.096533d, 0.088243d. The
KW    Aur    brightness varies with the orbital period.
KX    Aur    In the nebula IC 405.
KY    Aur    In the nebula IC 405.
LW    Aur    VB A (B 17.5m, 9", 46deg, 1999).
LY    Aur    d =  0.017P, Min II =  7.23 .
LY    Aur    VB A (B 9.154m Hp, 0.6", 253deg, 1991).
MN    Aur    Min II = 11.16 .
MN    Aur    P varies, current elements are given.
MR    Aur    Min II = 15.5.
MT    Aur    d =  0.02 P.
NQ    Aur    VB A (B 12.8m, 17", 143deg, 1999).
NU    Aur    Blazhko effect.
NV    Aur    OH, SiO, H2O maser.
NW    Aur    In the open cluster NGC 1893.
NX    Aur    In the open cluster NGC 1893.
OP    Aur    In the region of the open cluster Stock 8.
OX    Aur    VB A (B 10.2m, G5V(n), 22", 224deg, 1998). Multiperiodic.
OX    Aur    P0 is tabulated. P1 = 0.115442d.
OZ    Aur    Min II = 13.8  .
QT    Aur    VB A (B 15.8mV, 10", 266deg, 2000).
QU    Aur    VB A (B 6", 199deg, 1999).
QY    Aur    SB2, Porb = 10.4265d.
QZ    Aur    Eclipses outside the outburst: 16.98m - 18.95mV,
QZ    Aur    Min = 2448555.1595 + 0.3574961d x E [N0193].
V0348 Aur    VB A (B 12.8m V, 25", 222deg, 2007).
V0353 Aur    The protoplanetary nebula "Red Rectangle". The star was
V0353 Aur    brightening for several decades, between 1940s and 1970s.
V0355 Aur    Min II = 11.38 .
V0356 Aur    Multiperiodic, P2 = 0.15642d.
V0358 Aur    In the region of the open cluster NGC 2099.
V0361 Aur    Multiperiodic, P = 273s is dominating.
V0365 Aur    Min II = 14.2 :.
V0373 Aur    SiO maser.
V0382 Aur    [Fe/H] = -1.6.
V0386 Aur    [Fe/H] = -1.75.
V0387 Aur    [Fe/H] = -1.40.
V0388 Aur    Min II = 17.2 :.
V0390 Aur    VB (A 7.25m Hp; B 9.10m Hp, 0.4", 80deg, 1991). Accoring to
V0390 Aur    [N0197], also exhibits flares with amplitudes up to 0.29m U.
V0394 Aur    VB A (B F7V, 10.72m, 9", 209deg, 2007).
V0397 Aur    SB1, Porb > 1000d.
V0398 Aur    VB A (B 12.2m, 5", 82deg, 1958). Multiperiodic, P2 = 2.89404d.
V0402 Aur    Min II =  8.98 .
V0403 Aur    Porb = 83.1d.
V0404 Aur    Amplitude(Min II) = 0.28mag:.
V0404 Aur    Porb = 0.1726d.
V0406 Aur    Min II =  7.57 .
V0410 Aur    P varies, current elements are given.
V0411 Aur    The HD catalogue identifies HD 32447 (K) with BD+30 775, which
V0411 Aur    is V0411 Aur. In the HDE Atlas, V0411 Aur = HD 282867 (M0), and
V0411 Aur    HD 32447 (F2) is a different star.
V0417 Aur    Min II =  8.08 .
V0424 Aur    Min II =  8.44 .
V0424 Aur    VB (0.25", 229deg, 1998).
V0425 Aur    Min II =  7.84 .
V0426 Aur    Min II = 10.66 .
V0431 Aur    In the region of the open cluster NGC 1960.
V0432 Aur    d =  0.03 P.
V0432 Aur    One of the components probably pulsates.
V0433 Aur    SB?
V0437 Aur    The HIPPARCOS observations can be represented with several
V0437 Aur    different periods, the tabulated one contradicts later
V0437 Aur    observations.
V0440 Aur    ADS 4443A (B 12.0mV, 14", 15deg, 2000).
V0449 Aur    Min II =  7.53 .
V0455 Aur    Min II =  7.64 .
V0459 Aur    Min II =  7.96 .
V0462 Aur    Min II =  8.30 .
V0462 Aur    ADS 5582A (B 9.76m, 8", 210deg, 1991).
V0468 Aur    Min II = 12.6  .
V0469 Aur    VB B (A = V499 Aur; AB 25", 87deg, 1999).
V0490 Aur    VB.
V0495 Aur    Min II = 12.85 .
V0499 Aur    VB A (B = V469 Aur, 25", 87deg, 1999).
V0501 Aur    SB.
V0523 Aur    Min II = 14.1  .
V0528 Aur    SiO maser.
V0530 Aur    SiO maser.
V0534 Aur    Min II = 10.75 .
V0535 Aur    Min II = 13.15 .
V0539 Aur    In the open cluster M37 (NGC 2099). Probably non-member.
V0540 Aur    In the open cluster M37 (NGC 2099).
V0541 Aur    In the open cluster M37 (NGC 2099).
V0542 Aur    In the open cluster M37 (NGC 2099). The depth of MinII is 0.3m.
V0543 Aur    In the open cluster M37 (NGC 2099). The depth of MinII is 0.66m.
V0544 Aur    In the open cluster M37 (NGC 2099). The depth of MinII is 0.31m.
V0545 Aur    In the open cluster M37 (NGC 2099). Non-member?
V0546 Aur    In the open cluster NGC 2166. Type RS with P = 1.64470d is possible.
V0547 Aur    In the open cluster NGC 2166. Probably non-member.
V0548 Aur    In the open cluster NGC 2166. Probably non-member.
V0549 Aur    In the open cluster NGC 2166.
V0550 Aur    In the open cluster NGC 2166.
V0551 Aur    Min II = 14.58 .
V0551 Aur    In the open cluster NGC 2166. Delta Scuti variations: amplitude 0.05m, P = 0.12936d.
V0552 Aur    The period is for small-amplitude variations,
V0552 Aur    flickering is also observed; the combined amplitude of these
V0552 Aur    variations is 0.03m.
V0560 Aur    Min II =  9.18:.
V0560 Aur    VB (A 9.2m; B 9.6m, 0.9", 37deg, 1991).
V0562 Aur    Min II = 13.19 .
V0565 Aur    Min II = 12.16 .
V0567 Aur    Min II = 13.10 .
V0574 Aur    VB A (B 15.0mV, 11", 72deg, 2000).
V0576 Aur    Min II =  9.97:.
V0579 Aur    Min II = 14.35 .
V0579 Aur    VB A (B 15.4mV, 8", 133deg, 1999).
V0580 Aur    Min II = 13.8 :.
V0581 Aur    Originally erroneously named FS Boo, at a wrong position.
V0584 Aur    VB AB (10.1m, 11.4m, 0.5", 272deg, 2002).
V0585 Aur    Min II = 11.30.
V0589 Aur    Min II = 12.3.
V0591 Aur    Min II = 10.99.
V0594 Aur    Min II = 13.1.
V0596 Aur    Min II = 12.27.
V0599 Aur    Min II = 12.25.
V0603 Aur    Min II = 13.4. VB AB (5", 59deg, 1999).
V0606 Aur    Min II = 10.84.
V0607 Aur    Min II = 11.1.
V0608 Aur    Amplitude(Min II)=  0.15mag. VB A (B 15.8m, 9", 118deg, 2000).
V0609 Aur    Min II = 13.3.
V0610 Aur    Min II = 10.85 :.
V0612 Aur    Min II = 13.7 :.
V0617 Aur    Min II = 8.13. VB AB (8.27mHp, 11.42mHp, 1.2", 184deg, 1991).
V0618 Aur    Min II = 13.25.
V0620 Aur    Min II = 12.3.
V0622 Aur    Min II = 15.3 :.
V0623 Aur    Min II = 12.7.
V0624 Aur    A twice longer period is not excluded.
V0625 Aur    Min II = 17.36.
V0626 Aur    Min II = 15.83.
V0627 Aur    Min II = 14.05.
V0628 Aur    Min II = 15.99.
V0629 Aur    Min II = 16.75.
V0630 Aur    Min II = 14.22.
V0631 Aur    Min II = 16.59.
V0632 Aur    Min II = 16.35.
V0634 Aur    Min II = 15.22.
V0636 Aur    Min II = 13.91.
V0637 Aur    VB A (B 11.6mV, 14", 286deg, 2007).
V0639 Aur    Min II = 14.70.
V0640 Aur    Min II = 13.12.
V0641 Aur    Min II = 13.65.
V0644 Aur    Min II = 11.53.
V0645 Aur    Min II = 10.10. MinII - MinI = 0.789: x P.
V0646 Aur    Min II = 13.76.
V0647 Aur    Intermediate polar. Porb = 201min, Pspin = 1008.3408s or 930.5829s.
V0648 Aur    Min II = 11.80.
bet   Aur    Min II =  1.98 .
bet   Aur    VB A (C 14.1m, 13", 174deg, 1934).
eps   Aur    d =  0.04 P.
eps   Aur    VB A (B 14.0m, 30", 225deg, 2008; C 11.3m, 43", 276deg, 2008;
eps   Aur    D 12.0m, 45", 316deg, 2008). Probably eclipses are caused by
eps   Aur    a gas and dust disk. Besides eclipses, quasi-periodic brightness
eps   Aur    variations with an amplitude of several tenths of a magnitude
eps   Aur    and a cycle of 105 - 120 days (e.g., [N0204]). More rapid
eps   Aur    variations were also reported.
zet   Aur    d =  0.04 P.
zet   Aur    D = 0.041P, d = 0.038P (varies?).
tet   Aur    VB A (B 7.2m, 4", 306 deg, 2008).
psi 1 Aur    P1 = 150 - 200d, P2 = 2000d.
R     Boo    H2O maser.
V     Boo    Biperiodic, P1 = 137d. A long-term amplitude decrease.
V     Boo    SiO maser.
Z     Boo    H2O, SiO, OH maser.
RS    Boo    P varies, current elements are given. Possible Blazhko
RS    Boo    effect periods: 533d, 58d, 62d [04832]. [Fe/H] = -0.36.
RU    Boo    [Fe/H] = -1.50.
RX    Boo    P2 = 304.7d, possibly P3 = 2692d. H2O, SiO, OH maser.
SS    Boo    The depth of MinII is 0.1m, the distortion wave ampitude
SS    Boo    is up to 0.2m.
ST    Boo    [Fe/H] = -1.76. Blazhko effect, Pi = 284d [07238].
SU    Boo    Min II = 12.04 .
SU    Boo    P varies, current elements are given.
SV    Boo    [Fe/H] = -1.55.
SW    Boo    [Fe/H] = -1.12. P varies, current elements are given.
SY    Boo    Min II = 12.46:.
SZ    Boo    [Fe/H] = -1.68.
TU    Boo    Min II = 12.17 .
TU    Boo    P varies, current elements are given.
TV    Boo    [Fe/H] = -2.44.
TW    Boo    [Fe/H] = -1.46. P varies, current elements are given.
TX    Boo    Min II = 12.3  .
TX    Boo    P varies, current elements are given.
TY    Boo    Min II = 11.92 .
TY    Boo    P varies, current elements are given.
TZ    Boo    Min II = 10.82 .
TZ    Boo    P varies, current elements are given. Magnitudes in the minima
TZ    Boo    vary, sometimes MinII becomes deeper than MinI.
UU    Boo    P varies, current elements are given.
UW    Boo    P varies, current elements are given. The depth of MinII is
UW    Boo    0.1m pg.
UY    Boo    P varies.
VW    Boo    Min II = 10.93 .
VW    Boo    P varies, current elements are given.
XY    Boo    Min II = 10.73 .
XY    Boo    P varies, current elements are given.
YY    Boo    Min II = 12.1  .
ZZ    Boo    Min II =  7.44 .
AC    Boo    Min II = 10.67 .
AC    Boo    P varies, current elements are given.
AC    Boo    The light curve shape varies.
AD    Boo    Min II =  9.85 .
AE    Boo    [Fe/H] = -1.39.
AK    Boo    Min II = 16.3  .
AO    Boo    P varies, the mean P is given.
AQ    Boo    Min II = 12.9  .
AR    Boo    Min II = 13.5  .
AR    Boo    P varies, current elements are given.
BE    Boo    P varies?
BI    Boo    In the region of the globular cluster NGC 5466.
BK    Boo    In the region of the globular cluster NGC 5466.
BL    Boo    V19 (NGC 5466), cluster member. [Fe/H] = -1.92. P varies.
BN    Boo    In the region of the globular cluster NGC 5466.
BO    Boo    Blazhko effect.
BR    Boo    [Fe/H] = -1.03.
BU    Boo    Blazhko effect?
BW    Boo    Min II =  7.17 .
BW    Boo    MinII - MinI = 0.45P (1991).
BX    Boo    VB A (B 9.6m, 35", 156deg, 2007).
CC    Boo    z = 0.172.
CD    Boo    z = 1.045.
CE    Boo    Multiple.
CK    Boo    Min II =  9.22 .
CK    Boo    P varies, current elements are given.
CK    Boo    The light curve shape varies.
CM    Boo    [Fe/H] = -1.48.
CV    Boo    Min II = 11.36 .
DE    Boo    Porb = 125.4d.
DM    Boo    X-ray source.
DN    Boo    Min II = 11.28 .
DQ    Boo    VB AB (A 9.64m; B 10.92m, 9", 151deg, 1991).
DU    Boo    Min II =  8.86 .
DU    Boo    O'Connell effect.
DV    Boo    Min II =  7.69 .
DW    Boo    Min II =  7.43 .
EF    Boo    Min II =  9.78 .
EF    Boo    P varies, current elements are given.
EL    Boo    Min II =  9.42 .
EM    Boo    Min II =  9.23 .
EQ    Boo    Min II =  9.11 .
EQ    Boo    MinII - MinI = 0.399P. VB AB (A 9.4m; B 10.1m, 1.3", 271deg, 2005).
ET    Boo    Min II =  9.40 .
EW    Boo    Min II = 10.34 .
FI    Boo    Min II =  9.66 .
FL    Boo    VB AB (A 10.04m; B 10.37m, 7", 26deg, 1991).
FP    Boo    Min II = 10.38 .
FP    Boo    P varies? Current elements are given.
FS    Boo    Erroneously named at a wrong position because of a misprint. See V0581 Aur.
FY    Boo    Min II = 13.8  .
GG    Boo    Min II = 12.46 .
GH    Boo    Min II = 11.9  .
GI    Boo    Min II = 11.4  .
GK    Boo    Min II = 10.7  .
GL    Boo    Min II = 11.0  .
GM    Boo    Min II = 12.30 .
GM    Boo    P varies, current elements are given.
GN    Boo    P varies, current elements are given.
GO    Boo    Min II = 12.1 :.
GP    Boo    Min II = 10.75 .
GQ    Boo    Min II = 13.2  .
GQ    Boo    P varies, current elements are given.
GR    Boo    Min II = 11.80 .
GS    Boo    Min II = 11.45 .
GS    Boo    P varies, current elements are given.
GT    Boo    Min II = 12.3  .
GU    Boo    Min II = 13.7 :.
GV    Boo    Min II = 12.9  .
GV    Boo    P varies, current elements are given.
GW    Boo    Min II = 10.59 .
GX    Boo    Min II = 12.32 .
GX    Boo    Type DSCT with a twice shorter period is possible.
HH    Boo    Min II = 11.42 .
HK    Boo    SB2.
HQ    Boo    VB A (B 15.0mV, 24", 21deg, 1998). The tabulated amplitude can be influenced by the companion.
HR    Boo    Min II = 13.7  .
HW    Boo    Porb = 0.06435d.
IK    Boo    Min II = 11.69.
IL    Boo    Min II = 13.45.
IN    Boo    Min II = 14.3.
IO    Boo    Min II = 12.09. VB B (A 10.08m; AB 21", 93deg, 1999).
IP    Boo    P = 0.27596d is also possible.
IS    Boo    Min II = 14.5.
IW    Boo    Min II = 13.6.
IX    Boo    Min II = 13.15.
KK    Boo    Min II = 14.7.
KM    Boo    Min II = 14.6.
KN    Boo    P2 = 0.00157d.
KO    Boo    Min II = 13.35.
KP    Boo    Min II = 12.1.
KW    Boo    Min II = 14.5.
KZ    Boo    Min II = 13.1.
LL    Boo    P = 1.1708d is also possible.
LM    Boo    Min II = 13.1.
MN    Boo    Min II = 9.46. VB A (8.7mV; B 11.3mV, 10", 258deg, 2007).
MQ    Boo    Min II = 12.85.
MR    Boo    Min II = 11.34.
MT    Boo    Min II = 13.9.
MW    Boo    Min II = 14.4.
MY    Boo    Min II = 14.2.
NN    Boo    P1 is tabulated, P0 = 0.47462d.
NR    Boo    Min II = 14.2.
NT    Boo    Min II = 12.35.
NU    Boo    Min II = 13.75:.
NW    Boo    The depth of MinII is 0.18 mag.
NX    Boo    Min II = 13.36.
NY    Boo    Min II = 12.5.
NZ    Boo    Light elements for eclipses are tabulated. About 17.1m in quiescence, outside eclipses.
OP    Boo    Min II = 13.05.
OS    Boo    Min II = 14.0.
OT    Boo    Min II = 10.0.
OV    Boo    A cataclysmic-variable spectrum.
PR    Boo    Min II = 14.05.
PS    Boo    Min II = 12.5.
PT    Boo    Min II = 12.82.
PU    Boo    Min II = 10.85.
PY    Boo    Min II = 12.55.
PZ    Boo    Min II = 13.25. O'Connell effect.
QQ    Boo    Min II = 12.75.
QT    Boo    Min II = 11.75.
QV    Boo    Min II = 15.0.
QW    Boo    Min II = 12.4.
QX    Boo    Min II = 13.1.
QY    Boo    Min II = 12.85.
V0338 Boo    P0 is tabulated, P1 = 0.36691d.
V0339 Boo    Min II = 10.9.
gam   Boo    VB A (A speckle binary, 0.07", 78deg, 1975, unresolved on several other dates; B 12.7m, 48", 121deg, 1998).
kap 2 Boo    Multiperiodic. VB A (B 6.69m, F2V, SB1, 14", 237deg, 2009).
ksi   Boo    VB AB (4.73m, 7.04m, a = 4.9", Porb = 150 y).
i     Boo    Min II =  4.84 .
i     Boo    VB B (A = NSV 20241, 5.31m Hp, G0; B 6.09m Hp, a = 3.8", e = 0.43, Porb = 225 y); combined (A + B) magnitudes are tabulated.
i     Boo    P varies strongly, current elements are given.
R     Cae    SiO maser.
U     Cae    [Fe/H] = -1.11. Blazhko effect?
V     Cae    [Fe/H] = -2.00.
X     Cae    Multiperiodic.
RR    Cae    d = 0.02P.
RX    Cae    Variability type and spectral type do not agree.
RZ    Cae    VB (7.9m, 9.4m, 3", 222deg, 1993).
SX    Cae    A twice shorter period is also possible.
U     Cam    Triply periodic; other periods are 400d and 220d.
V     Cam    H2O, SiO maser.
Y     Cam    P varies, current elements are given. According to [N0223],
Y     Cam    MinI = 2424443.4806 + 3.30552340d x E + 0.1564d x sin(0.011052deg x E + 225.8deg) + 0.0452d x sim(0.022105 x E + 65.49deg).
Y     Cam    Superposed are pulsations with an amplitude up to 0.07m
Y     Cam    and P = 0.066457537d.
Z     Cam    Porb = 0.2898406d.
RR    Cam    Biperiodic; the other period is P0 = 223d.
RS    Cam    Triply periodic; other periods are 160d and 966d.
RT    Cam    H2O maser.
RU    Cam    [A/H] = 0.9. P varies. An unusual CWA variable with a carbon spectrum.
RU    Cam    In 1965, the star has abruptly changed the character of its variations,
RU    Cam    from nearly-regular, large-amplitude ones to mostly chaotic, with
RU    Cam    much smaller amplitude, sometimes decreasing to nearly zero.
RV    Cam    Multiperiodic. VB (0.07", 222deg, 1995) from speckle interferometry.
RX    Cam    SB, Porb = 1114d.
RY    Cam    VB (0.1", 350deg, 1997) from speckle interferometry.
RZ    Cam    [Fe/H] = -1.01.
SS    Cam    d = 0.06P. P varies, current elements are given.
ST    Cam    Triply periodic; other periods are 202d and 1580d.
SU    Cam    P varies, mean elements are given. Period variations have a
SU    Cam    possible period somewhat longer than 40 years.
SZ    Cam    ADS 2984B (A 6.93m; AB 18", 305deg, 2008). A very complex multiple star;
SZ    Cam    for component identifications see [N0228]. In the open cluster
SZ    Cam    NGC 1502. P varies, current elements are given.
TW    Cam    [Fe/H] = -0.8.
TX    Cam    VB A (B 16.6mpg, 8" nf). SiO maser.
UU    Cam    P varies, current elements are given.
UY    Cam    [Fe/H] = -1.33.
WW    Cam    MinII - MinI = 0.495P.
XX    Cam    Only one deep minimum near JD 2429632. No strong IR excess.
XX    Cam    P = 36:d in maximum [N0230].
AF    Cam    Porb = 0.2306d.
AG    Cam    SiO maser.
AH    Cam    VB A (B 14.32m, 7", 35deg, 1999). P varies, current elements are given.
AH    Cam    Blazhko effect with P = 11.0d [00232].
AK    Cam    P varies, current elements are given.
AL    Cam    P varies, current elements are given.
AO    Cam    P varies, current elements are given.
AS    Cam    d = 0.02P. DII = 0.06P. MinII - MinI = 0.437P. Long-period apsidal motion.
AS    Cam    Third body, P = 805d. According to [N0236], pulsations with
AS    Cam    P = 0.913d and amplitude 0.02m are observed outside minima.
AX    Cam    VB (Porb = 6.644y, a = 0".554, e = 0.660).
AY    Cam    d = 0.02P.
BD    Cam    SB1, Porb = 596d.
BL    Cam    Multiperiodic; P varies [N0237].
BM    Cam    SB1, Porb = 80.1745d, e = 0.35.
BT    Cam    Multiperiodic. P2 = 0.0079d, other periods.
BW    Cam    H2O, OH maser.
BX    Cam    H2O, SiO, OH maser.
BY    Cam    Other detected periods: 7.3d; 145d.
BZ    Cam    In a nebula.
CE    Cam    SB?
CH    Cam    The central star of the planetary nebula NGC 1501. Multiperiodic.
CI    Cam    A single strong outburst in 1998. According to [N0245],
CI    Cam    multiperiodic pulsations are observed outside the outburst,
CI    Cam    the dominating periods being 0.41521d and 0.26647d.
CI    Cam    Porb = 19.407d.
CL    Cam    SB1, Porb = 20.8d.
CM    Cam    SB1, Porb = 3770d.
CS    Cam    VB A (B 8.22m, 2", 164deg, 1991).
CS    Cam    doubt which of the components varies.
CV    Cam    VB AB (9.80m, 10.84m, 4", 44deg, 1991).
CZ    Cam    The detected semiregular variations are not typical of the spectral type.
DL    Cam    VB A (B 6.96m, 10", 308deg, 1991).
DM    Cam    VB AaAb (7.82m, 8.10m, 0".1, 170deg, 1991).
FH    Cam    Alternatively, can be a pulsating star with a twice shorter period.
FT    Cam    Porb = 0.074990d.
GS    Cam    VB A (8.39mJ, Sp C; B 12.09mJ, 23", 219deg, 2000). There remains
HT    Cam    Porb = 0.060d.
IQ    Cam    Biperiodic. Second periodicity: P = 0.3248d.
LL    Cam    SiO maser.
LQ    Cam    SiO maser.
LS    Cam    Porb = 0.143d.
LU    Cam    Porb = 0.15d.
LW    Cam    Porb = 0.06754658d.
MM    Cam    Chromospherically active giant, slow photometric variations.
MU    Cam    The orbital period is tabulated. The spin period from photometry is 0.01374127d.
MW    Cam    Biperiodic, P2 = 0.1282d.
NR    Cam    O'Connell effect.
R     Cnc    OH, H2O, SiO maser.
S     Cnc    In the region of the open cluster NGC 2632 (Praesepe). P varies?
T     Cnc    SiO maser.
U     Cnc    In the region of the open cluster NGC 2632 (Praesepe).
V     Cnc    VB A (B 13.7m, 9", 276deg, 2002).
W     Cnc    H2O, SiO maser.
X     Cnc    Other periods suspected. SB?, Porb = 491.4:d.
Y     Cnc    Blazhko effect.
RS    Cnc    Multiperiodic, P2 = 128.760d. H2O, SiO maser.
RW    Cnc    Blazhko effect periods: 29.9d, 91.1d [02088]. [Fe/H] = -1.67.
RY    Cnc    In the region of the open cluster NGC 2632 (Praesepe). P varies, current elements are tabulated.
SS    Cnc    [Fe/H] = -0.07.
SW    Cnc    P varies?
SY    Cnc    Porb = 0.38d.
SZ    Cnc    SiO maser.
TT    Cnc    P varies, current elements are tabulated. Blazhko effect, P = 89.3d. [Fe/H] = -1.57.
TU    Cnc    P varies, current elements are tabulated.
TX    Cnc    In the open cluster NGC 2632 (Praesepe). P varies, current elements are tabulated.
TY    Cnc    P varies, current elements are tabulated.
UV    Cnc    In the region of the open cluster NGC 2632 (Praesepe).
VZ    Cnc    P2 = 0.142804d. Beat period: 0.716292d.
WW    Cnc    P varies, current elements are tabulated.
WY    Cnc    VB A (B+C 12.5m; B 25", 356deg, 1998; C 28", 1deg, 1998). P varies, current elements are tabulated.
XX    Cnc    In the region of the open cluster NGC 2632 (Praesepe).
YZ    Cnc    Porb = 0.0868d.
AC    Cnc    Physical variations, additional minima were reported.
AE    Cnc    VB A (B 15.5m, 11", 18deg, 2000).
AF    Cnc    Blazhko effect, P = 27.23d.
AG    Cnc    In the region of the open cluster NGC 2682 (M 67). SB2, Porb = 2.823094d.
AH    Cnc    P varies, quadratic term +1.56d x 10^(-10) x E^2. In the open cluster NGC 2682 (M 67), probable member.
AK    Cnc    Porb = 0.0651d.
AN    Cnc    [Fe/H] = -1.45.
AO    Cnc    P varies?
AP    Cnc    Blazhko effect?
AR    Cnc    The period tabulated is for eclipses that occur, in quiescence, from the V = 18.7 level.
AS    Cnc    [Fe/H] = -1.89.
AT    Cnc    Surrounded with a filamentary nebula, which is presumably a Nova remnant.
AU    Cnc    In the open cluster NGC 2632 (Praesepe).
AV    Cnc    In the open cluster NGC 2632 (Praesepe).
AW    Cnc    In the open cluster NGC 2632 (Praesepe).
AX    Cnc    In the open cluster NGC 2632 (Praesepe).
AY    Cnc    In the open cluster NGC 2632 (Praesepe).
AZ    Cnc    In the open cluster NGC 2632 (Praesepe).
BB    Cnc    In the open cluster NGC 2632 (Praesepe).
BC    Cnc    In the open cluster NGC 2632 (Praesepe).
BD    Cnc    In the open cluster NGC 2632 (Praesepe).
BE    Cnc    In the open cluster NGC 2632 (Praesepe).
BF    Cnc    VB A (B 16.7mV, 9", 37deg, 2000). Blazhko effect?
BG    Cnc    In the open cluster NGC 2632 (Praesepe).
BM    Cnc    SB, Porb = 585.4154d.
BN    Cnc    In the open cluster NGC 2632 (Praesepe). Multiperiodic.
BO    Cnc    P2 = 270d.
BQ    Cnc    Multiperiodic. SB2. In the open cluster NGC 2632 (Praesepe).
BR    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BS    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BT    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BU    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BV    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BW    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BX    Cnc    Multiperiodic. In the open cluster NGC 2632 (Praesepe).
BY    Cnc    In the open cluster NGC 2632 (Praesepe).
BZ    Cnc    In the open cluster NGC 2632 (Praesepe).
CC    Cnc    Porb = 0.07352d. In the region of the open cluster NGC 2632 (Praesepe).
CD    Cnc    In the open cluster NGC 2632 (Praesepe).
CE    Cnc    In the open cluster NGC 2632 (Praesepe).
CF    Cnc    In the open cluster NGC 2632 (Praesepe).
CG    Cnc    In the open cluster NGC 2632 (Praesepe).
CH    Cnc    In the open cluster NGC 2632 (Praesepe).
CI    Cnc    In the open cluster NGC 2632 (Praesepe).
CK    Cnc    In the open cluster NGC 2632 (Praesepe).
CL    Cnc    In the open cluster NGC 2632 (Praesepe).
CM    Cnc    In the open cluster NGC 2632 (Praesepe).
CN    Cnc    In the open cluster NGC 2632 (Praesepe).
CO    Cnc    In the open cluster NGC 2632 (Praesepe).
CP    Cnc    In the open cluster NGC 2632 (Praesepe).
CR    Cnc    In the open cluster NGC 2632 (Praesepe).
CS    Cnc    In the open cluster NGC 2632 (Praesepe).
CU    Cnc    VB A (B = CV Cnc, 10", 348deg, 2001, common proper motion). In the region of the open cluster NGC 2632 (Praesepe), non-member. Eclipses: 11.67 - 11.82V, MinII 11.75V, D = 0.03P, Min = 2450208.5068 + 2.771468d x E [N0335].
CV    Cnc    VB Bab (0.8", 200deg, 2006; A = CU Cnc, AB 10", 348deg, 2001, common proper motion). In the region of the open cluster NGC 2632 (Praesepe), non-member.
CW    Cnc    H2O maser.
CY    Cnc    In the open cluster NGC 2632 (Praesepe).
DD    Cnc    In the open cluster NGC 2632 (Praesepe).
DF    Cnc    In the region of the open cluster NGC 2632 (Praesepe), non-member?
DG    Cnc    In the region of the open cluster NGC 2632 (Praesepe), non-member?
DH    Cnc    In the open cluster NGC 2632 (Praesepe).
DI    Cnc    In the open cluster NGC 2632 (Praesepe).
DK    Cnc    In the region of the open cluster NGC 2632 (Praesepe).
DL    Cnc    In the open cluster NGC 2632 (Praesepe).
DM    Cnc    In the open cluster NGC 2632 (Praesepe).
DN    Cnc    In the open cluster NGC 2632 (Praesepe).
DO    Cnc    In the open cluster NGC 2632 (Praesepe).
DP    Cnc    In the open cluster NGC 2632 (Praesepe).
DQ    Cnc    In the region of the open cluster NGC 2632 (Praesepe), non-member?
DR    Cnc    In the open cluster NGC 2632 (Praesepe).
DS    Cnc    In the region of the open cluster NGC 2632 (Praesepe), non-member?
DT    Cnc    In the open cluster NGC 2632 (Praesepe).
DU    Cnc    In the open cluster NGC 2632 (Praesepe).
DY    Cnc    In the open cluster NGC 2632 (Praesepe).
DZ    Cnc    In the open cluster NGC 2632 (Praesepe).
EE    Cnc    In the open cluster NGC 2632 (Praesepe).
EG    Cnc    Porb = 0.05997d.
EH    Cnc    P varies, current elements are tabulated.
EI    Cnc    VB AB (1.4", 77deg, 2005).
EL    Cnc    In the open cluster NGC 2632 (Praesepe).
EM    Cnc    In the open cluster NGC 2632 (Praesepe).
EN    Cnc    In the open cluster NGC 2632 (Praesepe).
EO    Cnc    In the open cluster NGC 2632 (Praesepe).
EP    Cnc    Multiperiodic. In the region of the open cluster NGC 2632 (Praesepe).
EQ    Cnc    In the open cluster NGC 2632 (Praesepe).
ER    Cnc    In the open cluster NGC 2632 (Praesepe).
ES    Cnc    In the region of the open cluster NGC 2682 (M 67).
ET    Cnc    In the open cluster NGC 2682 (M 67).
EU    Cnc    In the open cluster NGC 2682 (M 67).
EV    Cnc    O'Connell effect. A blue straggler in the open cluster NGC 2682 (M 67).
EW    Cnc    Multiperiodic. A blue straggler in the open cluster NGC 2682 (M 67).
EX    Cnc    Multiperiodic. A blue straggler in the open cluster NGC 2682 (M 67).
EY    Cnc    In the open cluster NGC 2682 (M 67).
FL    Cnc    Multiperiodic.
FM    Cnc    Blazhko effect?
FN    Cnc    Blazhko effect, P = 50.3d?
FP    Cnc    VB A (B 12.3mV, M3, 14", 240deg, 2004).
FV    Cnc    In the open cluster NGC 2632 (Praesepe). SB2, Porb = 2.981781d.
GS    Cnc    VB A (12.5mV; B 12.7mV, 10", 267deg).
GY    Cnc    Eclipses of different depth, from all all outburst brightness levels. The light elements for eclipses are tabulated.
GZ    Cnc    Porb = 0.08825d.
HI    Cnc    In the open cluster NGC 2632 (Praesepe).
HK    Cnc    Multiperiodic.
HM    Cnc    Two white dwarfs on a very-short-period orbit.
HN    Cnc    P varies, current elements are tabulated.
HO    Cnc    VB AB (9.62m, 9.76m, 3", 1deg, 2011).
HP    Cnc    VB AB (9.91m, 10.09m, 1.4", 168deg, 2010).
HQ    Cnc    In the open cluster NGC 2682 (M 67), non-member.
HR    Cnc    In the open cluster NGC 2682 (M 67).
HS    Cnc    The light curve shape varies. In the open cluster NGC 2682 (M 67).
HT    Cnc    Porb = 1.358766d. In the open cluster NGC 2682 (M 67).
HU    Cnc    SB1, Porb = 18.396d. In the open cluster NGC 2682 (M 67).
HV    Cnc    In the open cluster NGC 2682 (M 67).
HW    Cnc    SB2, Porb = 10.05525d. In the open cluster NGC 2682 (M 67).
HX    Cnc    SB, Porb = 2.66059. In the open cluster NGC 2682 (M 67).
HY    Cnc    In the open cluster NGC 2682 (M 67).
HZ    Cnc    Multi-mode pulsations at a time scale of hours.
IO    Cnc    P varies?
KK    Cnc    VB (the NW component varies). Superhumps: P = 0.060818d.
KQ    Cnc    Blazhko effect?
KV    Cnc    Blazhko effect, P = 42d:.
KZ    Cnc    In the region of the open cluster NGC 2682 (M 67).
LN    Cnc    In the region of the open cluster NGC 2682 (M 67). Type RRC with a twice shorter period is also possible.
LO    Cnc    In the region of the open cluster NGC 2682 (M 67), probably non-member.
LP    Cnc    In the region of the open cluster NGC 2682 (M 67).
LT    Cnc    Pulsations at a timescale of about an hour. SB, Porb = 6.1163d.
LV    Cnc    Multiperiodic, P2 = 0.0025d. SB, Porb = 0.0567d. Cataclysmic spectrum.
kap   Cnc    SB, P = 6.39616d.
R     CVn    OH, SiO maser.
U     CVn    OH, H2O maser.
V     CVn    Multiperiodic, P2 = 186d. OH, H2O, SiO maser.
W     CVn    [Fe/H] = -1.22. P varies, current elements for 1999 are tabulated. Quadratic elements: Max = 2421402.421 + 0.55175963d x E -0.4156d x 10^{-10}E^2 [N0347].
Y     CVn    Multiperiodic, other periods: 273d, 160d.
Z     CVn    [Fe/H] = -1.98. P varies, elements valid after 1999 are tabulated. Blazhko effect, P = 22.75d.
RR    CVn    [Fe/H] = -1.08.
RS    CVn    d = 0.033P. P varies, current elements are tabulated. Distorsion wave: Delta(m) from 0.09m to 0.20m, P = 4.7917d [07209].
RU    CVn    [Fe/H] = -1.38. P varies, current elements are tabulated.
RV    CVn    V141 (M3 = NGC 5272), cluster non-member. P varies, current elements are tabulated.
RX    CVn    [Fe/H] = -1.31.
RZ    CVn    [Fe/H] = -1.84.  P varies, current elements are tabulated.
SS    CVn    [Fe/H] = -1.37. P varies? Blazhko effect?
ST    CVn    [Fe/H] = -1.07.
SV    CVn    [Fe/H] = -2.20. P varies, current elements are tabulated.
SW    CVn    P varies, quadratic term +2.0334d x 10^{-10}E^2. [Fe/H] = -1.53.
TX    CVn    Porb = 199.0:d.
UU    CVn    In the region of the globular cluster NGC 5466. P varies, current elements are tabulated. Blazhko effect?
UV    CVn    In the region of the globular cluster NGC 5466; cluster non-member. P varies, current elements are tabulated.
UW    CVn    In the region of the globular cluster NGC 5466.
UZ    CVn    [Fe/H] = -1.89. P varies, current elements for Hipparcos observations are tabulated.
VW    CVn    P varies, current elements for 1999 are tabulated. The light curve shape varies?
WW    CVn    Blazhko effect.
WY    CVn    V205 (M3 = NGC 5272).
WZ    CVn    V206 (M3 = NGC 5272). Blazhko effect, P = 25.4d?
XX    CVn    V113 (M3 = NGC 5272).
XY    CVn    [Fe/H] = -2.03.
XZ    CVn    [Fe/H] = -1.46. P varies strongly, elements for JD 2455939 - 2456462 are tabulated.
YY    CVn    P varies strongly, elements for JD 2455939 - 2456462 are tabulated.
AA    CVn    [Fe/H] = -1.78.
AC    CVn    Blazhko effect.
AD    CVn    [Fe/H] = -1.39. VB A (B 16.0mV, 10", 147deg, 1998).
AF    CVn    [Fe/H] = -1.19.
AG    CVn    [Fe/H] = -2.01.
AH    CVn    [Fe/H] = -1.93.
AI    CVn    Multiperiodic.
AK    CVn    [Fe/H] = -1.62.
AM    CVn    Multiperiodic; also Min = 2448742.5610 + 0.011906623d x E (presumably orbital variations) and other periods. The tabulated period (double wave) can be interpreted as positive superhumps. Often considered a system of two white dwarfs.
AN    CVn    [Fe/H] = -1.54.
AP    CVn    VB A (13.6mV; B 13.9mV, 23", 183deg, 2000).
AQ    CVn    A probable field horizontal-branch star. A single strong brightening, about 20 minutes duration, was observed.
BD    CVn    Blazhko effect?
BF    CVn    VB A (B = NSV 6039, 13.16m, dM3.5e, 16", 226deg, 1991). Flares in the combined light of the pair (Delta U up to 0.95m) were observed [02195].
BG    CVn    Multiperiodic. Also P = 780s (0.00903d), etc.; different periods dominate at different times.
BI    CVn    P varies, current elements are tabulated.
BM    CVn    SB, Porb = 20.625d. Somewhat different periods were observed during different seasons of observations.
BN    CVn    P varies, quadratic term +1.7372d x 10^{-10}E^2.
BO    CVn    P varies, current elements are tabulated.
CH    CVn    SB.
CP    CVn    SB.
CS    CVn    HIPPARCOS data are in contradiction with the M0V spectral type.
CU    CVn    Multiperiodic.
CX    CVn    VB (A 9.5mHp, B 13.2mHp, 1.3", 308deg, 1991).
DD    CVn    Multiperiodic.
DE    CVn    EA-like in U and B light, EB at longer wavelengths. Amplitude decreases with wavelength.
DG    CVn    VB (Delta(mK) = 0.16m, 0.17", 253deg, 2000).
DK    CVn    The light curve shape varies strongly.
DN    CVn    P varies strongly [00001].
DY    CVn    P varies, current elements are tabulated. VB A (B 15m, 5", 250deg, 1998).
DZ    CVn    Blazhko effect.
EF    CVn    P varies?
EG    CVn    P varies, current elements are tabulated.
EI    CVn    P varies?
FL    CVn    Blazhko effect?
FT    CVn    Blazhko effect.
FV    CVn    P varies, current elements are tabulated.
alf 2 CVn    Epoch of Max is tabulated. VB A (2.81mHp; B 5.86mHp, 19", 229deg, 1991).
R     CMa    P varies, current elements are tabulated.
Y     CMa    SiO maser.
Z     CMa    Speckle interferometry: VB (0.1", 305deg, 1993).
RR    CMa    P varies, current elements are tabulated.
RT    CMa    P varies, current elements are tabulated.
RX    CMa    P varies.
RZ    CMa    P varies? Current elements are tabulated.
SS    CMa    P varies? Current elements are tabulated.
SW    CMa    MinII - MinI = 0.31P. e = 0.32.
SY    CMa    VB A (companions: 7", 156deg; 14", 270deg, 1994).
TT    CMa    SiO maser.
UU    CMa    P varies, current elements are tabulated.
UZ    CMa    Multiperiodic, P2 = 38.4d.
VY    CMa    In the region of the young open cluster NGC 2362. Embedded in a reflecting nebula. ADS 6033 A; numerous companions are probably details of the nebula. H2O, OH, SiO maser.
AO    CMa    In the region of the open cluster Ruprecht 18.
AS    CMa    d = 0.04P.
BG    CMa    VB (5", 20deg, 1999). The variable is probably the southern component.
BQ    CMa    In the region of the open cluster NGC 2354.
CE    CMa    MinII - MinI = 0.663P.
CG    CMa    VB A (B 16m, 4", 261deg, 1999).
CN    CMa    [Fe/H] = 0.0.
CV    CMa    Currently, MinII - MinI = 0.46P. Apsidal motion.
DL    CMa    OH maser.
DM    CMa    No red star near the published position. Cataclysmic? [00001].
DS    CMa    VB A (B 15.8m, 9", 320deg, 1998).
DZ    CMa    The elements for fundamental mode are tabulated. P1 = 1.64495d.
EW    CMa    VB (4.920mHp, 5.394mHp, 0.131", 324deg, 1991). SB, P = 0.261975d. Shell events. BCEP-like variations, P = 0.0918d [N0367]. Other reported periods: about 20d [N0366], 1.2572d [N0367].
EY    CMa    Multiperiodic.
EZ    CMa    SB. In the ring nebula S308. In the region of the open cluster Collinder 121. P2 = 1.18d was possible in 1988.
FF    CMa    In the region of the open cluster Collinder 132a.
FN    CMa    VB (A 5.685mHp; B 7.042mHp, 0.571", 116deg, 1991; C 9.0mV, B6V, 18", 350deg, 2011). The range in the table is for the A+B pair. Associated with the nebula vB 95. The period needs confirmation.
FR    CMa    VB (A 5.55mV; B 9.7mV, 4", 23deg, 2003).
FU    CMa    VB Aab (6.52m, 0.1", 337deg, 2010; B 11,07m, 14", 232deg, 1999).
FV    CMa    VB AB (5.7mV, 7.7mV, 0.1", 11deg, 2012).
FZ    CMa    In the HII region S 295.
GG    CMa    In the open cluster Cr 132a.
GU    CMa    VB AB (7.03m, 7.70m, 0.6", 198deg, 1991). In the HII region S 293.
HK    CMa    In the region of the open cluster NGC 2287.
HL    CMa    Probably related to XM variables. The X-ray source 1E 0643.0-1648. Lx/Lopt is from 0.002 to 1. Porb = 0.2145d.
HN    CMa    Multiperiodic.
HP    CMa    Several possible periods or cycles were reported. VB A (B 8.21m, 5", 220deg, 1999).
HQ    CMa    VB A (B 13.0m, 9", 220deg, 1999).
HW    CMa    Orbital eccentricity e = 0.500.
II    CMa    In the region of the open cluster Be 33.
IK    CMa    In the open cluster Be 33.
IL    CMa    Pulsation periods (unstable) of 1.19d and 1.28d were reported.
IU    CMa    VB (6.85m, 8.15m, 0.8", 156deg, 1991).
IY    CMa    VB (5.86mV, 7.60mV, 1.2", 43deg, 1999).
KL    CMa    Apsidal motion. MinII = 2448.171.228 + 1.762168d x E. VB A (B 10.47m, 21", 43deg, 2011).
KQ    CMa    VB A (B 11.29mV, 7", 42deg, 1999).
KY    CMa    Mean brightness varies with P2 = 493d.
LT    CMa    Apsidal motion. MinII = 2448389.445 + 1.759503d x E.
LX    CMa    P = 4.362d according to [HIP].
MX    CMa    In the region of the open cluster NGC 2362.
NN    CMa    Semiperiodic bursts (P = 210d).
NO    CMa    In the region of the open cluster Cr 140.
NQ    CMa    VB (9.9mV, 13.2mV, 5", 64deg, 1999).
NS    CMa    In the region of the open cluster NGC 2243.
NT    CMa    In the region of the open cluster NGC 2243.
NU    CMa    In the region of the open cluster NGC 2243.
NV    CMa    In the region of the open cluster NGC 2243.
NW    CMa    In the region of the open cluster NGC 2243.
NX    CMa    In the region of the open cluster NGC 2243.
PX    CMa    In the region of the open cluster Tombaugh 2.
PY    CMa    In the region of the open cluster Tombaugh 2.
PZ    CMa    In the region of the open cluster Tombaugh 2.
QQ    CMa    In the region of the open cluster Tombaugh 2.
QR    CMa    In the region of the open cluster Tombaugh 2.
QS    CMa    In the region of the open cluster Tombaugh 2.
QT    CMa    VB A (B 9", 252deg, 2000).
QU    CMa    In the region of the open cluster NGC 2354.
QX    CMa    Type EW is also possible. In the open cluster NGC 2362.
V0347 CMa    VB A (B 13.5m, 8", 92deg, 1998). The tabulated magnitude at maximum is influenced by the companion.
V0350 CMa    Multiperiodic, P2 = 0.7750d. VB A (6.332mHp; B 8.895mHp, 18", 144deg, 1991).
V0356 CMa    VB AB (2", 22deg, 2001; C 10.8m, 14", 116deg, 1999).
V0367 CMa    Superposed variations with an amplitude up to 0.5m and a period of 89d.
V0377 CMa    A twice shorter period is not excluded.
V0388 CMa    VB (9.1m, 9.1m, 3", 330deg, 1991). MinII - MinI = 0.61P.
V0400 CMa    In the open cluster NGC 2204.
V0401 CMa    In the open cluster NGC 2204.
V0402 CMa    In the open cluster NGC 2204.
V0403 CMa    In the open cluster NGC 2204.
V0404 CMa    P varies, dP/dt = -0.47 x 10^(-5) d/yr.
V0406 CMa    In the open cluster NGC 2243.
V0407 CMa    In the open cluster NGC 2243.
V0408 CMa    In the open cluster NGC 2243.
V0409 CMa    Type EW with a twice longer period is also possible. In the open cluster NGC 2243.
V0410 CMa    In the open cluster NGC 2243.
V0411 CMa    In the open cluster NGC 2243.
V0412 CMa    In the open cluster NGC 2243.
V0413 CMa    In the open cluster NGC 2243.
V0415 CMa    VB A (B 9.3m, 9", 335deg, 1999).
V0416 CMa    P varies, dP/dt = 0.27 x 10^(-5) d/yr.
V0422 CMa    In the open cluster NGC 2362.
bet   CMa    Multiperiodic.
iot   CMa    Non-radial pulsations?
tau   CMa    VB Aa, Ab (4.89mV, 5.33mV, 0.1", Porb = 154.9d; B 10.2mV, 9", 93deg, 2002; C 11.2mV, 14". 87deg, 2002; E 9.7mV, Ab-E 0.9", 88deg, 2012).
ome   CMa    P = 1.3719d in radial velocities was reported.
R     CMi    SC4/10e.
T     CMi    P var. Max = 2422456 + 324.2d*E (JD2416610 -
T     CMi    22800); Max = 2430896 + 311.2d*E (JD2423090 -
T     CMi    30900); since JD2430900 - see Table.
U     CMi    There is a hump on the ascending branch looking sometimes
U     CMi    as a secondary maximum. The light curve for 1904 - 1970
U     CMi    [07368].
X     CMi    P var? Delta(S) = 3.
RS    CMi    d = 0.02P:.
RX    CMi    Min II 14.6; Min II - Min I = 0.52P:.
RY    CMi    Min II 12.0:.
SX    CMi    DI <= 0.12P. Min II 13.6.
SY    CMi    P var. Max = 2425234.682 + 0.565900d*E (JD2425234 - 708);
SY    CMi    since JD2436586 - see Table.
TU    CMi    Min II 15.1.
TW    CMi    Min II 15.6.
TX    CMi    Min II 14.7.
UZ    CMi    Min II 12.1.
XZ    CMi    Min II 9.88. P var?
YY    CMi    Min II 8.88.
YZ    CMi    mu = 0.604", P = 221.4deg. Epoch of Min is given. P var;
YZ    CMi    additional term: -0.00003919514d*E*(E + 1)/2. Periodical
YZ    CMi    light variations with the amplitude 0.12m (11.26 - 11.38 V)
YZ    CMi    are superimposed by strong flares.
AG    CMi    P var. Min = 2434698.670 + 1.6645729d*E (JD2426350 -
AG    CMi    34740) [01727]. Since JD2437650 - see Table.
AH    CMi    EW?
AK    CMi    Min II 10.3; Min II - Min I = 0.55P. P var. Min I =
AK    CMi    2425352.348 + 0.56589534d*E (JD2424880 -
AK    CMi    35550) [01728]. Since JD2435600 - see Table.
AL    CMi    Observations in the interval JD2424880 - 25950 are
AL    CMi    represented by the elements: Max = 2425243.631 + 0.55050d*E.
AL    CMi    Since JD2436590  -  see Table.
AM    CMi    Min II 10.5.
AN    CMi    d = 0.02P:.
AO    CMi    d = 0.01P:. Min II 14.5.
BF    CMi    Depth of Min II 0.05m:.
BO    CMi    Several episodes of outburst-like activity.
CX    CMi    MinII 11.97.
DL    CMi    A twice shorter period is not excluded.
DO    CMi    Multiperiodic. P0 is tabulated, P1 = 0.14862d, P2 = 0.11908d, P3 = 0.11617d.
DP    CMi    Min II = 10.78:.
DR    CMi    Min II = 11.42. MinII - MinI = 0.67P.
DS    CMi    Min II = 11.88.
DW    CMi    The depth of MinII is 0.7 mag (*).
DX    CMi    Min II = 12.1 :.
DY    CMi    Superhumps: P = 0.060750d.
EG    CMi    Min II = 13.7.
EI    CMi    Min II = 13.8.
EK    CMi    Min II = 12.20.
EL    CMi    Min II = 12.1.
EP    CMi    Min II = 12.9.
EQ    CMi    Min II = 13.5.
RS    Cap    Mean brightness varies with P = 3360d.
RT    Cap    VB A (B 15m, 26", 227deg).
RU    Cap    VB A (B 13.6m, 1.6", 86deg).
RV    Cap    P var: Max = 2424334.6612 + 0.44775262d*E
RV    Cap    (JD2417400 - 33610) [00323]. Since JD2433850 - see Table.
RV    Cap    Light curve and period vary with the Blazhko effect
RV    Cap    period Pi = 225.5d [06464]. Semiamplitude  of deviations
RV    Cap    from linear elements is +-0.032d. 0.14P <= M - m <= 0.25P.
RV    Cap    (k - b)2 = 0.05.
RW    Cap    d = 0.020P. Min II 9.9. P var. Min I  = 2418924.594 +
RW    Cap    3.3923922d*E (JD2418920 - 24000) [06774];
RW    Cap    Min I  = 2424003.014 + 3.3923457d*E (JD2424000 -
RW    Cap    34500) [02389]; since JD2435400 - see Table.
RX    Cap    Min II 12.5.
RY    Cap    VB B (A 7.1m, F0; B 6.6", 90deg; C 12.0m, 8.5", 58deg).
TV    Cap    P = 67d [01331].
TW    Cap    P var. P = 28.6421871d (JD2414000 - 17600);
TW    Cap    P = 28.61700115d (JD2417600 - 24000) [01331];
TW    Cap    Max = 2426211.90 + 28.59497d*E (JD2421400 -
TW    Cap    26200) [02390]; Max = 2435664.8 + 28.5578d*E
TW    Cap    (JD2426210 - 37500) [02309]; since JD2437500 - see Table.
TW    Cap    0.14P <= M - m <= 0.40P. [Fe/H] =  -0.72.
TY    Cap    Min II 10.6. P var. Min I hel = 2432017.956 + 1.423466D*E
TY    Cap    (JD2425500 - 35000); since JD2435000 - see Table.
UW    Cap    Min II 11.5; Min II - Min I = 0.5P. P var? Min I =
UW    Cap    2434627.290 + 1.399118d*E (JD2427000 - 35000);
UW    Cap    since JD243500 - see Table.
YZ    Cap    (k - b)2 = 0.08.
AD    Cap    Outside eclipses B - V =  +1.00. P var?
AE    Cap    Mean brightness varies with P = 2300d.
BH    Cap    Type RR: is also possible.
BN    Cap    The variability may be due to the fainter (B) component.
CM    Cap    MinII 10.20.
CR    Cap    The first-overtone period is tabulated. P0 = 0.47203d, Delta(m)1/Delta(m)0 = 1.5.
DK    Cap    Multiperiodic.
DM    Cap    Porb = 0.2215d.
del   Cap    VB A (B 15.8m, 69", 94deg; C 12.7m, 119", 302deg,
del   Cap    1911); mu = 0.391", P = 138.8deg. Min II 2.90.
del   Cap    The light curve shape var? [03305].
eps   Cap    VB A (B 9.52m, 68.7", 47deg).
R     Car    VB A (B 12m, 2.1", 138deg). H2O, SiO maser.
U     Car    P var. Max = 2429023.80 + 38.753d*E (JD2415000 -
U     Car    29500); since JD2429500 - see Table.
V     Car    The light curve shape var?
X     Car    Min II 8.6.
Y     Car    VB A (B 12.22m, 15"; C 12.96m, 30"). SB (P = 400 - 600d)
Y     Car    [05119]. The fundamental mode period P0 is given in the
Y     Car    Table (A = 0.58m). The first overtone period P1 = 2.55954d
Y     Car    [05119] (A = 0.28m). P1/P0 = 0.7032.
RR    Car    P var. P = 154d (JD2421500 - 23500); P = 259d
RR    Car    (JD2426400 - 30100); P = 154d (JD2430400 - 33100).
RR    Car    S6.5/1- .
RT    Car    In the region of the cluster Tr 15.
RY    Car    There is a close companion 14.3 pg. P var.
RY    Car    Max = 2418475 + 416d*E (JD2415140 - 18500);
RY    Car    Max = 2429901 + 417.3d*E (JD2423600 - 32900);
RY    Car    since JD2434100 - see Table.
ST    Car    Depth of Min II 0.27m.
SW    Car    Depth of Min II 0.05m.
SZ    Car    In the region of the cluster NGC 3114.
TX    Car    The light curve shape var?
TZ    Car    Mean brightness varies with P = 1183d; the amplitude of
TZ    Car    the short cycle is large in mean brightness maximum and
TZ    Car    small during its minimum.
UX    Car    In the region of the cluster IC 2581.
VV    Car    In the region of the very poor cluster N 99 [07374]
VV    Car    (10h 36.0m -58deg 56', 1950.0) embedded in a nebula.
VY    Car    VB A (B 11.07m; B 9V:, 10", 150deg). P var.
VY    Car    Nonlinear term: -0.000021d*E**2 (JD2410000 - 44200).
VY    Car    The latest observations may be represented also by linear
VY    Car    elements: Max = 2444161.16 + 18.9138d*E
VY    Car    (JD2441000 - 44200). [A/H] = 0.4.
WZ    Car    P var. Max = 2419981.099 + 23.000945d*E (JD2410000 - 20000)
WZ    Car    [00025]; Max = 2423984.12 + 23.0054d*E (JD2419800 - 25500)
WZ    Car    [00322]; Max = 2434914.86 + 23.0075d*E + 0.000025d*E**2
WZ    Car    (JD2434500 - 41200) [02309]; since JD2434500 - see also
WZ    Car    Table.
XX    Car    P var. Max = 2420769.703 + 15.723704d*E (JD2410000 - 22500)
XX    Car    [00025]; P = 15.7196d (JD2423000 - 30000) [00003]; since
XX    Car    JD2434500 - see Table; elements given in the Table contain
XX    Car    a nonlinear term: -0.0000034d*E**2.
XY    Car    [A/H] = 0.1.
XZ    Car    [A/H] = 0.2.
YZ    Car    P var. Nonlinear term: +0.0000022d*E**2. [A/H] = -0.1.
AE    Car    In the region of the cluster NGC 3532.
AF    Car    P var. Max = 2434532 + 433.7d*E (JD2420200 - 34600); since
AF    Car    JD2435000 - see Table.
AG    Car    Central star of the low-excitation planetary nebula
AG    Car    P.K.289-0.1 ejected probably during a nova-like outburst
AG    Car    of the star about 1000 years ago [07052, 07113].
AS    Car    d = 0.025P.
AW    Car    d = 0.015P.
BL    Car    In the region of the cluster Tr 16.
BO    Car    VB A (B 11.05m V, B8III, 10", 41deg). In the region of
BO    Car    the cluster Tr 15. Cluster non-member.
BP    Car    P = 4.82246d?
BS    Car    In the region of the cluster IC 2602. Min II 15.3.
BU    Car    Min II = 13.9.
BZ    Car    Mean brightness possibly varies with P = 1800d.
CD    Car    In the centre of the cluster Cr 236.
CF    Car    In the region of the cluster NGC 3496.
CH    Car    VB A (B 8", 194deg, 2000).
CI    Car    In the region of the cluster NGC 3572. d = 0.021P?
CO    Car    d = 0.024P?
CV    Car    d = 0.046P. Depth of Min II 0.05m.
DE    Car    d = 0.016P?
DH    Car    VB B (A 15.2m V; B 13", 350deg). B - V = +0.90m
DH    Car    (Min brightness).
DI    Car    Besides Cepheid-like light variations with the amplitude
DI    Car    1.7m and elements Max = 2438553.70 + 29.210d*E
DI    Car    (JD2438465 - 40300) [05324] large weakenings of brightness
DI    Car    are observed [04678]. At Max B - V = +1.34.
DK    Car    d = 0.07P.
DM    Car    d = 0.040P.
DP    Car    d = 0.034P. Min II 13.1.
DS    Car    d = 0.03P.
DU    Car    In the region of the cluster IC 2602.
DW    Car    In the region of the cluster Cr 228. Min II 10.3.
EF    Car    d = 0.04P.
EG    Car    In the region of the cluster NGC 3532.
EH    Car    VB A (B 15", 320deg).
EK    Car    In the region of the cluster NGC 3532.
EM    Car    Min II 8.9.
EN    Car    In the region of the cluster Tr 18.
EQ    Car    d = 0.030P. Min II 13.7.
ER    Car    In the region of the cluster NGC 3532.
ES    Car    In the region of the cluster NGC 3572.
EZ    Car    Min II 9.8.
FI    Car    P var. Max = 2425446.81 + 13.4542d*E (JD2423790 - 35300)
FI    Car    [00046, 02309]. Since JD2435300 - see Table.
FK    Car    VB.
FO    Car    VB A (B 14m, 7", 90deg). P var. Max = 2434922.531 +
FO    Car    10.3559d*E (JD2423700 - 35300) [06006]; since JD2436000
FO    Car    - see Table. B - V: +1.13, +1.43.
FP    Car    d = 0.01P:.
FQ    Car    In the region of the cluster Tr 18.
FS    Car    In the region of the very poor cluster N 99 [07374] (10h
FS    Car    36.0m -58deg 56', 1950.0) embedded in a nebula. Min II
FS    Car    10.9.
FT    Car    According to [02197] spectrum C. Misidentification is
FT    Car    possible.
FV    Car    VB A (B 13m, 10", 135deg). P var. There are two additional
FV    Car    terms in the elements given in the Table:
FV    Car    -0.1065d*10**(-7)*E**2 - 0.584d*10**(-11)*E**3.
FV    Car    d = 0.02P:. Min II 13.0.
GG    Car    Min II 9.5. Gas and dust envelope.
GH    Car    In the region of the cluster Tr 18.
GK    Car    In the region of the cluster Tr 19. Min II 13.2.
GL    Car    In the region of the cluster NGC 3572. Min II 10.31.
GL    Car    System with the apsidal motion; e = 0.157, omega = 99deg.
GL    Car    There are sinusoidal terms in the elements for Min I given
GL    Car    in the Table: +0.121d sin(0.094389deg*E) -
GL    Car    0.007d sin(0.188778deg*E);
GL    Car    Min II = 2424263.236 + 2.4222338d*E -
GL    Car    0.121d sin(0.094389deg*E) - 0.007d sin(0.188778deg*E).
GL    Car    DII = 0.17P.
GM    Car    In the region of the very poor cluster N 99 [07374] (10h
GM    Car    36.0m -58deg 56', 1950.0) embedded in a nebula.
GM    Car    Min II 9.22.
GN    Car    Min II 12.1.
GO    Car    VB A (B 15", 60deg).
GP    Car    Min II 12.8.
GQ    Car    Min II 13.5.
GR    Car    Min II 14.0; Min II - Min I = 0.316P; DII = 0.05P.
GV    Car    Possible member of the cluster NGC 3532. Min II 9.1.
GW    Car    Min II 9.9.
GZ    Car    Light elements for the fundamental mode oscillation with
GZ    Car    an amplitude 0.16m are given in the Table. For the first
GZ    Car    overtone oscillation with an amplitude 0.07m
GZ    Car    Max = 2440742.4 + 2.93424d*E. Epochs of maxima and
GZ    Car    amplitudes are given according to [05175].
HH    Car    VB A (B 13.0m, 5", 260deg; C 11.11m, 13", 337deg; D 12.65m,
HH    Car    15", 7deg). d = 0.02P. Min II 10.66. P var [08094].
HH    Car    Min I hel = 2430860.162 + 3.2315393d*E (JD2427590 - 35260)
HH    Car    [05292]. Possible current elements are given in the Table.
HI    Car    Min II 10.8.
HK    Car    VB A (B 12.5m, 4"). Range of combined brightness variation
HK    Car    is given.
HL    Car    d = 0.03P:.
HN    Car    Min II 12.5.
HP    Car    VB A (B 9.1m, 0.4", 178deg). Min II 9.3. Elements should
HP    Car    be corrected [08083].
HQ    Car    B - V: +0.63,  +1.04.
HR    Car    Spectrum description  [01914, 06466].
HT    Car    In the region of the cluster IC 2581. Min II 14.0.
HV    Car    d = 0.026P. Min II 14.2.
HW    Car    Epoch of Min is given.
HX    Car    Min II 14.5.
IK    Car    In the region of the cluster NGC 2602.
IL    Car    Min II 14.4.
IN    Car    It is possible that the period must be doubled.
IQ    Car    In the region of the cluster NGC 3532.
IR    Car    In the region of the cluster NGC 3532. Min II 12.6.
IS    Car    Min II 14.0.
IU    Car    (k - b)2 = 0.02.
IW    Car    Mean brightness varies with the period close to 1500d, the
IW    Car    amplitude of main oscillations - from 1.3m to 0.3m.
IX    Car    In the centre of a bright nebula with the diameter 2.4'.
IZ    Car    Declination in [00085] is wrong by 3deg. Identical to
IZ    Car    V336 Car, see [06316].
KQ    Car    Min II 10.3.
KU    Car    Min II 11.6.
MP    Car    VB A (B 16m, 180deg).
MZ    Car    sf component of a close pair.
OO    Car    Min II 14.7.
OV    Car    Min II 13.5.
OY    Car    Eclipse elements:
OY    Car    Min I hel = 2443993.553241 + 0.0631209247d*E [05185];
OY    Car    D = 0.050P, d = 0.044P. The hump on the light curve is
OY    Car    observed at the phase of 0.75P. Depth of Min I varies
OY    Car    between 1.48m and 2.47m.
PT    Car    Min II 13.0:.
PX    Car    Min II 10.10.
QR    Car    Min II 10.4.
QS    Car    Min II 9.3.
QU    Car    HDE 310376 (HA 112, 173). Flickering resembles V818 Sco.
QU    Car    Variations by 0.2m in 90s were observed. No periodicity
QU    Car    was found. Emission lines He II 4686, CIV - NIII 4630 -
QU    Car    4650 and sometimes weak hydrogen absoptions (corresponding
QU    Car    to A or B type) are noticeable in the spectrum [05643].
QX    Car    Min II 7.02.
QY    Car    In the open cluster No.90 [07374].
QZ    Car    In the eta Carina nebula, possible member of the cluster
QZ    Car    Collinder 228. Min II 6.43. Two SB1 systems (A and B),
QZ    Car    B is eclipsing (A: SB1, P = 20.73d, O9.5 I,
QZ    Car    Delta(m) = 0.6m). Combined brightness is given.
V0341 Car    In the variable reflecting nebula IC 2220. In the region
V0341 Car    of the open cluster NGC 2516. IR excess.
V0343 Car    VB. SB (P = 133.92d).
V0347 Car    Deep Min II.
V0348 Car    In the open cluster IC 2581. Min II 8.9.
V0354 Car    Very red.
V0356 Car    Member of the cluster NGC 2516.
V0357 Car    SB (P = 6.74483d [04627]).
V0361 Car    In the region of the cluster NGC 3293.
V0365 Car    In the region of the cluster NGC 3532.
V0367 Car    Min II 7.54.
V0373 Car    Member of the cluster NGC 2516.
V0374 Car    Member of the cluster NGC 2516.
V0375 Car    P = 0.264d or 0.359d.
V0376 Car    VB A (B 6.83m, B 9.5V, 41", 75deg).
V0378 Car    In the open cluster NGC 3293.
V0379 Car    In the open cluster NGC 3293.
V0380 Car    In the open cluster NGC 3293.
V0381 Car    In the open cluster NGC 3293.
V0382 Car    In the region of the cluster NGC 3532.
V0384 Car    The mean brightness varies, P = 790d. Originally [08741], a neighbor (GSC9196.00400} was annonced as the variable, while the true var. stars was used a comparison star.
V0385 Car    Depth of Min II 0.04m. Surrounded by a ring nebula RCW 58.
V0491 Car    Mean magnitude 9.69.
V0493 Car    SB, Porb = 3.368d.
V0498 Car    Type BE: is also possible.
V0534 Car    Flare-like activity.
V0575 Car    MinII 8.08.
V0576 Car    Almost monotone brightening during 12 years.
V0592 Car    MinII 11.45.
V0598 Car    MinII 11.32.
V0607 Car    In the region of the open cluster NGC 2516.
V0621 Car    VB A (B 14.6m, 12", 347deg, C 15.2m, 5", 27deg, 2000).
V0625 Car    Period varies [205].
V0627 Car    VB A (B 13.5mpg, 22", 18deg, 1998).
V0638 Car    VB A (B 15.1mpg, 6", 27deg, 2000).
V0644 Car    Double-peaked maxima.
V0655 Car    MinII - MinI = 0.38P.
V0660 Car    In the Eta Carinae Nebula. VB A (B 10.8mV, 21", 206deg, 1998), the tabulated magnitude at maximum can be influenced.
V0661 Car    MinII - MinI = 0.65P. In the Eta Carinae Nebula. VB A (B 12.5m, 12", 158deg, 2000).
V0662 Car    In the Eta Carinae Nebula.
V0665 Car    A twice shorter period is not excluded.
V0674 Car    MinII - MinI = 0.29P. Multiple (faint companions).
V0675 Car    VB A (B 12.2mR, 6", 20deg, 1996).
V0680 Car    VB B (A 7.74m, A0V; AB 17", 238deg, 1998).
V0681 Car    Min II = 10.19. Light elements for eclipses are tabulated. Pulsations with P = 0.214292d and amplitude about 0.03m.
V0684 Car    Min II = 8.94. VB AB (A 9.03m; B 10.70m, 4", 188deg, 1941).
V0686 Car    Min II = 9.01.
V0701 Car    P0 is tabulated, P1 = 2.869d. VB AB (11.44m, 11.66m, 0.9", 1991).
V0706 Car    The mean brightness varies with a cycle about 1900d.
V0712 Car    Min II = 11.07.
V0713 Car    Min II = 9.62.
V0714 Car    Min II = 9.77.
V0717 Car    Min II = 10.85. Besides variations with the tabulated period, a second EB periodicity is revealed, P2 = 1.110270d, with amplitudes 0.20m (primary) and 0.15m (secondary).
V0718 Car    Min II = 10.85. Besides variations with the tabulated period, a second EW periodicity is revealed, P2 = 0.388607d, with amplitudes of both minima about 0.1m.
V0720 Car    VB A (A 10.38m var; B 10.62m, 16", 53deg, 1991). Combined magnitudes are tabulated.
V0724 Car    VB A (B 13.2m, 4", 80deg, 1934).
V0725 Car    Min II = 10.05. MinII - MinI = 0.16P.
V0731 Car    Min II = 9.7. VB A (B 9.61m, 27", 2deg, 1991; C 9.64m, 15", 195deg, 1991.
V0733 Car    Min II = 10.91.
V0734 Car    Min II = 11.30. MinII - MinI = 0.44P.
V0736 Car    Min II = 8.17. MinII - MinI = 0.655P.
V0738 Car    Min II = 9.14.
V0744 Car    Min II = 8.49.
V0750 Car    SB3.
V0754 Car    SB3.
V0772 Car    Min II = 8.07.
V0788 Car    SB2, a triple system.
V0790 Car    SB2, a triple system.
V0802 Car    Mean brightness varies. VB A (B 11.7m, 5", 222deg, 2000).
V0821 Car    SB3.
V0829 Car    Min II = 9.51.
V0831 Car    Min II = 7.78. Possibly also an intrinsic variable.
V0833 Car    Min II = 9.54.
eta   Car    In the emission nebula NGC 3372 in the region of the
eta   Car    cluster Tr 16. A very massive young star surrounded by an
eta   Car    expanding gas and dust shell with the diameter 2" at 2mu
eta   Car    and 6.5" at 12.2mu. Maximum brightness was observed in
eta   Car    1843. Since 1880 varies in the range 5.9 - 7.9 V. In the
eta   Car    interval JD2434000 - 41000 Max = 2434037 + 1110d*E. There
eta   Car    are emission lines of H, HeI, FeII, [FeII], etc. in the
eta   Car    spectrum. Description of the spectrum [05251, 07279].
eta   Car    Soft X-ray source of variable intensity.
khi   Car    Soft X-ray source.
R     Cas    VB A (B 14.5m, 14", 273deg). SiO, OH maser;
R     Cas    sometimes H2O emission.
T     Cas    SiO maser. ZrO bands in the infrared spectral region.
U     Cas    S4.5/4e.
W     Cas    SC5/9e.
X     Cas    P var: Max = 2426650 + 432.32d*E (JD2416750 - 27060);
X     Cas    Max = 2432870 + 413.6d*E (JD2427060 - 32870);
X     Cas    Max = 2437948 + 423.0d*E (JD2432870 - 39210).
X     Cas    Current elements are given in the Table.
Y     Cas    OH, H2O emission; SiO maser.
Z     Cas    SiO maser.
RS    Cas    P var. Max = 2416942.16 + 6.29552d*E (JD2412650 - 34900)
RS    Cas    [03317]. Since JD2434900 - see Table.
RV    Cas    There are signs of Se type in the spectrum [03383].
RW    Cas    P var. Max = 2421354.22 + 14.8004d*E (JD2417000 - 30000).
RW    Cas    Since JD2430000 - see Table. [A/H] = 0.3.
RX    Cas    Unigue rapidly evolving eclipsing system. 9.12<=Min II<=9.49;
RX    Cas    Min II - Min I = 0.5070P. P var. Nonlinear term:
RX    Cas    +1.017d*10**(-5)*E**2. Observations may be represented
RX    Cas    also by three systems of elements: Min I =
RX    Cas    2416250.889 + 32.31481d*E (0 <= E <= 286,
RX    Cas    JD2416250 - 25482); Min I = 2416248.835 + 32.32145d*E
RX    Cas    (331 <= E <= 554, JD2426940 - 34155);
RX    Cas    Min I = 2416244.990 + 32.32765d*E (734 <= E <= 876,
RX    Cas    JD2439970 - 44570). Brightness of the system out of
RX    Cas    eclipses periodically varies within 8.6m - 9.0m with
RX    Cas    elements Max = 2416198 + 516.06d*E [05036]. Max - Min =
RX    Cas    233d = 0.45P [00881]. Strong emissions of H, NV, CIV,
RX    Cas    SIIV, FeIII. Powerful gaseous stream and accretion
RX    Cas    phenomena are possible.
RY    Cas    [A/H] = 0.0.
RZ    Cas    Min II 6.26. The light curve shape var; d var
RZ    Cas    (0.000P <=  d <= 0.009P). P var, variations are irregular.
RZ    Cas    Mean elements based on visual and photographic
RZ    Cas    observations: Min I = 2416886.8806 + 1.195253065d*E
RZ    Cas    (JD2416800 - 26700) [08820], Min I = 2432820.7853 +
RZ    Cas    1.1952517d*E (JD2426700 - 34000) [00938]. From
RZ    Cas    photoelectric observations: Min I = 2432115.5827 +
RZ    Cas    1.1952472d*E (JD2429870 - 30400); Min I =
RZ    Cas    2432085.7011 + 1.195259d*E (JD2432000 - 32460);
RZ    Cas    Min I = 2434349.5130 + 1.1952525d*E (JD2432450 - 34420);
RZ    Cas    Min I = 2434703.3035 + 1.195238d*E (JD2434420 - 34705);
RZ    Cas    Min I = 2435934.4087 + 1.1952499d*E (JD2434705 - 35950);
RZ    Cas    Min I = 2438829.2818 + 1.195243d*E (JD2436800 - 39100);
RZ    Cas    Min I = 2440182.3089 + 1.195259d*E (JD2439380 - 40200);
RZ    Cas    Min I = 2441333.3257 + 1.195244d*E (JD2440500 - 41350);
RZ    Cas    Min I = 2442327.7798 + 1.1952521d*E (JD2441550 - 42350);
RZ    Cas    since JD2442850 - see Table.
SU    Cas    [A/H] = -0.1.
SV    Cas    P var. Max = 2421839 + 279.3d*E (JD2417600 -
SV    Cas    21900); Max = 2430450 + 281.7d*E (JD2422500 -
SV    Cas    31900); since JD2432600 - see Table.
SX    Cas    VB A (B 11.5m, 19", 250deg, 1966). Min II 9.32. The light
SX    Cas    curve shape var. DII = 0.171P:, dI = 0.036P, dII = 0.050P.
SX    Cas    P var. Min I = 2433963.267 + 36.56727d*E (JD2418000 -
SX    Cas    37000); since JD2438700 - see Table. Strong emissions
SX    Cas    of H, NV, CIV, SIIV, FeIII. Gaseous streams and accretion
SX    Cas    phenomena.
SY    Cas    VB? P var. Max = 2417911.547 + 4.070969d*E
SY    Cas    (JD2417000 - 34000); since JD2434000 - see Table.
SZ    Cas    P var. Max = 2421261.66 + 13.6009d*E (JD2416700 - 21260);
SZ    Cas    Max = 2426650.20 + 13.6072d*E (JD2421260 - 27170) [08821];
SZ    Cas    Max = 2429727.240 + 13.61744d*E (JD2427170 - 33050);
SZ    Cas    Max = 2436810.92 + 13.62655d*E (JD2433050 - 38720);
SZ    Cas    since JD2438720 - see Table. [A/H] = -0.6.
TU    Cas    Fundamental mode period P0 is given in the Table; the
TU    Cas    corresponding amplitude is 0.69m. First-overtone period
TU    Cas    P1 = 1.51830d; the corresponding mean amplitude decreased
TU    Cas    from 0.4m to 0.25m during 67 years [05078]. P1/P0 = 0.71.
TU    Cas    M - m var (0.17P <=  M - m <= 0.35P).
TV    Cas    d = 0.01P. Min II 7.34. The light curve shape var.
TV    Cas    Period of these variations - 600d [08822]. P var. Mean
TV    Cas    elements based on visual and photographic observations:
TV    Cas    Min I = 2432827.7665 + 1.81260983d*E (JD2415650 - 32800)
TV    Cas    [01926]. From photoelectric observations Min I =
TV    Cas    2432827.7665 + 1.8126142d*E (JD2432800 - 36490);
TV    Cas    Min I = 2436483.8091 + 1.81255d*E (JD2436480 - 36980);
TV    Cas    Min I = 2438472.2386 + 1.81263d*E (JD2437000 - 38500);
TV    Cas    Min I = 2438829.3230 + 1.8126048d*E (JD2438470 - 41750);
TV    Cas    since JD2441750 - see Table.
TW    Cas    Min II 8.40.
TX    Cas    Min II 9.6.
TY    Cas    P var. Max = 2419260 + 545.0d*E (JD2419200 - 25300);
TY    Cas    Max = 2428965 + 623.8d*E (JD2427000 - 41500);
TY    Cas    since JD2441500 - see Table.
UU    Cas    Min II 10.5.
UZ    Cas    [A/H] = -0.3.
VV    Cas    P var. Max = 2422514.16 + 6.207510d*E (JD2417000 - 32500);
VV    Cas    since JD2432500 - see Table. [A/H] = -0.2.
VW    Cas    [A/H] = 0.0.
WY    Cas    In the region of the cluster NGC 7789.
WY    Cas    The spectrum of the G type star is seen in minimum light
WY    Cas    [03502]. The existence of a physical companion is possible.
WY    Cas    S6/6-e.
WZ    Cas    VB A (optical companion B 8.7m, 58", 89deg). SC7/10e.
WZ    Cas    Light variations are sometimes taking place with doubled
WZ    Cas    period.
XX    Cas    Min II 10.2.
YZ    Cas    VB A (B 11.23m, 35", 160deg). d = 0.045P. Min II 5.78.
ZZ    Cas    Min II 10.9.
AB    Cas    EA/SD. Min II 10.28. P var. Min I = 2430755.678 +
AB    Cas    1.366863d*E (JD2425400 - 33150); Min I =
AB    Cas    2433616.532 + 1.366876d*E (JD2433150 - 37000);
AB    Cas    Min I = 2440475.5216 + 1.3668783d*E (JD2437000 -
AB    Cas    41600); since JD2441600 - see Table.
AB    Cas    The A3 component is a DSCT type variable with the elements:
AB    Cas    Max hel = 2444912.1759 + 0.0582874d*E [08825]; amplitude
AB    Cas    of pulsations Delta(V) var (0.03m <= Delta(V) <= 0.09m).
AE    Cas    Min II 12.8.
AH    Cas    Min II 13.3.
AL    Cas    Min II 13.6.
AO    Cas    Min II 6.24. The light curve shape var. P var?
AQ    Cas    Min II 10.4.
AR    Cas    VB A (B 9.3m, 1.0", 336deg; C 8.2m, 75", 269deg;
AR    Cas    D 9.8m, 76", 268deg; E 11.28m, 43", 115deg; F 11.06m, 69",
AR    Cas    338deg; G 11.11m, 67", 348deg). Min II 4.86;
AR    Cas    Min II - Min I = 0.614P; DII = 0.076P; dII = 0.037P.
AS    Cas    VB A (B 15.5m, 3", 45deg).
AS    Cas    Fundamental mode period P0 is given in the Table; the
AS    Cas    corresponding amplitude is 0.59m. First-overtone period
AS    Cas    P1 = 2.2909d; amplitude of oscillations with this period
AS    Cas    is 0.13m. P1/P0 = 0.76.
AX    Cas    Min II 12.9.
AZ    Cas    B - V: +1.78, +2.20. D = 110d, d = 88d = 0.026P.
BD    Cas    B - V: +1.50, +1.61. P var. Max = 2429124.84 +
BD    Cas    3.65129d*E (JD2415000 - 29130) [00915];
BD    Cas    since JD2429130 - see Table.
BE    Cas    VB A (B G, 25", 260deg).
BM    Cas    Min II 8.98. Shape of the light curve varies. P var.
BM    Cas    There is a periodic term in the elements:
BM    Cas    +2.6d*sin(7.11deg*E + 104deg).According to [00939], on the
BM    Cas    light curve cepheid-like variations are observed with
BM    Cas    P = 27d.
BN    Cas    Min II 13.4.
BS    Cas    Min II 12.6.
BU    Cas    D = 0.02P.
BY    Cas    In the region of the cluster NGC 663. P var.
BY    Cas    Max = 2416871.91 + 3.2218d*E (JD2416800 - 24860) [00921];
BY    Cas    Max = 2431929.60 + 3.221297d*E (JD2426900 - 34300);
BY    Cas    Max = 2438399.629 + 3.222588d*E (JD2436200 - 39400);
BY    Cas    since JD2439400 - see Table.
BZ    Cas    Min II 11.5.
CC    Cas    Min II 7.26. The light curve shape var? P var?
CE    CasA   Possible member of the cluster NGC 7790. VB A (B = CEb Cas,
CE    CasA   2.4", 265deg).
CE    CasB   VB B (A = CEa Cas). Possible member of the cluster NGC 7790.
CF    Cas    Possible member of the cluster NGC 7790. [A/H] = 0.1.
CG    Cas    In the region of the cluster NGC 7790.
CH    Cas    [A/H] = -0.5.
CQ    Cas    The slow oscillations are superimposed by more rapid ones
CQ    Cas    with cycles from 110d to 250d.
CR    Cas    Min II 13.3.
CS    Cas    [A/H] = -0.4.
CV    Cas    Epochs given in [00922] are not represented by the elements
CV    Cas    given in the Table. P var?
CW    Cas    Min II 11.47. Shape of the light curve and depths of
CW    Cas    minima vary. P var. Min I = 2435745.6163 + 0.31886497d*E
CW    Cas    (JD2432400 - 41000) [03332]; since JD2441000 - see Table.
CY    Cas    [A/H] = -0.7.
DD    Cas    P var. Max = 2415612.45 + 9.807272d*E (JD2415600 - 18600);
DD    Cas    since JD2418600 - see Table. The star may be a member of a
DD    Cas    binary system with Porb = 8500d +- 1000d.
DF    Cas    In the region of the cluster NGC 1027.
DI    Cas    P var. Max = 2432068 + 371.7d*E (JD2417200 - 32100);
DI    Cas    since JD2432100 - see Table.
DL    Cas    Member of the cluster NGC 129. [A/H] = 0.0.
DN    Cas    Min II 10.13.
DO    Cas    Min II 8.61; dI = 0.08P.
DP    Cas    Min II 13.6.
DZ    Cas    Min II 12.0.
EG    Cas    Min II 13.1.
EK    Cas    Depth of Min II 0.05m.
EM    Cas    P var. Max = 2433132 + 283d*E (JD2427700 - 33150); since
EM    Cas    JD2433150 - see Table. Amplitude strongly varies.
EN    Cas    Min II 12.4. P var.
EP    Cas    Min II 11.4.
EQ    Cas    Min II 12.7. P var. Min I = 2432150.04 + 58.26d*E
EQ    Cas    (JD2432200 - 34060) [03336]; since JD2436100 - see Table.
EY    Cas    Min II 14.5.
GG    Cas    d = 0.013P. Min II 9.99. P var? Min I = 2430188.468 +
GG    Cas    3.758738d*E (JD2424800 - 39500) [00936];
GG    Cas    since JD2439500 - see Table.
GK    Cas    Depth of Min II 0.05m.
GT    Cas    d = 0.02P.
GU    Cas    Min II 11.3. P var. Min I = 2428749.423 + 3.093329d*E
GU    Cas    (JD2417470 - 35480) [00941];
GU    Cas    Min I = 2437367.375 + 3.09325d*E (JD2435480 - 38750) [00001];
GU    Cas    since JD2438750 - see Table.
GZ    Cas    Mean magnitude varies with P = 800d.
GZ    Cas    Max = 2428000 + 800d*E [00911].
HH    Cas    Epoch of Min is given. RV type is possible [00911].
HN    Cas    d = 0.038P.
HS    Cas    VB A (B 12m, 27", 15deg).
HT    Cas    Min hel = 2443727.93722 + 0.073647217d*E;
HT    Cas    D = 0.13P. Depth of eclipses between outbursts is ~2.4 V.
HT    Cas    Small quasi-periodic light oscillations with P = 100s.
HT    Cas    Spectrum description [06163].
HU    Cas    P var. Max = 2417525.075 + 0.41159875d*E (JD2411600 -
HU    Cas    28000); since JD2428000 - see Table.
IL    Cas    Depth of Min II 0.05m.
IR    Cas    Min II 11.5. P var. Min I = 2428750.2914 +
IR    Cas    0.68069178d*E (JD2417500 - 38400) [00098];
IR    Cas    since JD2438400 - see Table.
IS    Cas    Min II 12.2. P var. Min I = 2428776.262 +
IS    Cas    1.8415172d*E (JD2417400 - 29500) [00098];
IS    Cas    since JD2428000 - see Table.
IT    Cas    Min II 11.8; Min II - Min I = 0.553P; DII = 0.042P.
IT    Cas    Apsidal motion is possible.
IV    Cas    Min II 11.3. P var. Min I = 2428991.302 +
IV    Cas    0.9985232d*E (JD2416700 - 29000) [00098];
IV    Cas    Min I = 2431438.648 + 0.9985056d*E (JD2429000 -
IV    Cas    37700) [02263]; since JD2440000 - see Table.
IW    Cas    S4 +/6e.
IX    Cas    P var. Max = 2428749.39 + 9.15035d*E (JD2414700 -
IX    Cas    29500) [00098]; Max = 2428749.90 + 9.1363d*E
IX    Cas    (JD2428700 - 34350) [00944]; Max = 2437195.642 +
IX    Cas    9.14783d*E (JD2434350 - 39100) [05462];
IX    Cas    since JD2442000 - see Table. [A/H] = -0.4.
KL    Cas    Min II 12.3.
KO    Cas    P var. Max = 2425590 + 305.6d*E (JD2416700 - 26000);
KO    Cas    since JD2426000 - see Table.
KR    Cas    Min II 9.9.
LR    Cas    Min II 10.9.
LU    Cas    Min II 14.3?
LW    Cas    In the apex of a small (8") bright cometary nebula in the
LW    Cas    region of IC 1848. Novalike outburst was observed in the
LW    Cas    interval JD2433900 - 34800. Infrared and radioemission.
LX    Cas    In the region of the cluster Collinder 33. Min II 15.3;
LX    Cas    Min II - Min I = 0.47P; dI = 0.10P.
LY    Cas    In the region of the cluster Collinder 33. Min II 15.2.
MM    Cas    d = 0.08P: Min II 12.4.
MN    Cas    Min II 10.57.
MO    Cas    In the nebula NGC 7635. 10.2 - 13.1 I.
MP    Cas    In the nebula NGC 7635. 10.4 - 13.5 I.
MR    Cas    Min II 15.5.
MS    Cas    Min II 13.2.
MT    Cas    d = 0.04P. Min II 14.02.
MU    Cas    Min II 10.8.
MV    Cas    Min II 14.0.
MY    Cas    Min II 15.2. P var. Elements given in the Table are valid
MY    Cas    since JD2438500.
NN    Cas    Min II 14.0.
NT    Cas    Min II 14.4.
NU    Cas    Min II 13.4.
NV    Cas    d = 0.03P.
OP    Cas    P var. Max = 2429109.726 + 5.510019d*E (JD2427950 - 34670)
OP    Cas    [00176]; since JD2437000 - see Table.
OR    Cas    Min II 11.8. P var. Min I = 2429249.424 + 1.2457026d*E
OR    Cas    (JD2413800 - 34800) [00176]; since JD2432000 - see Table.
OX    Cas    In the region of the cluster NGC 381. d = 0.016P. Min II
OX    Cas    10.30; Min II - Min I = 0.512P. Apsidal motion [04524].
PR    Cas    P = 171d?
PV    Cas    Min II 10.36; Min II - Min I = 0.480P.
PV    Cas    Depth of Minima probably varies. P var. Min I =
PV    Cas    2428796.8142 + 1.75047346d*E (JD2415700 - 40000) [05302];
PV    Cas    since JD2440000 - see Table. Apsidal motion [06253]:
PV    Cas    Min II = 2428797.6894 + 1.75047346d*E -
PV    Cas    0.040d*sin(0.0075deg*(E - 3000)).
PX    Cas    Min II 15.0.
PY    Cas    Epoch of Min brighness is given. Similar to RV Tau by
PY    Cas    light curve shape [03348].
PZ    Cas    VB A (B 12.8m, WN 8:, 15", 100deg). OH, H2O emission.
QQ    Cas    Min II 10.8. P var. Min I = 2434330.169 + 2.142030d*E
QQ    Cas    (JD2415700 - 30000) [02530]; since JD2430000 - see Table.
QX    Cas    In the region of the cluster NGC 7790. VB A (B 13.1m, 3").
QX    Cas    Min II 10.50; Min II - Min I = 0.37P; DII = 0.047P;
QX    Cas    dII = 0.018P.
V0336 Cas    Min II 13.6.
V0341 Cas    d = 0.031P.
V0344 Cas    Min II 13.4.
V0345 Cas    Min II 13.6.
V0346 Cas    The coordinates refer to the sp component of a wide pair,
V0346 Cas    whereas the chart [02345] leads to the nf component. It is
V0346 Cas    the sp component that is red and probably var.
V0357 Cas    Min II 13.6.
V0359 Cas    Min II 12.0.
V0360 Cas    Min II 12.3.
V0361 Cas    d = 0.051P.
V0363 Cas    Delta(S) = 1.
V0364 Cas    Min II 11.9.
V0365 Cas    S6/3- .
V0366 Cas    Min II 12.7. P var. Min I = 2435075.461 + 0.7292714d*E
V0366 Cas    (JD2414600 - 35400) [02305]; since JD2434650 - see Table.
V0373 Cas    An unique close binary. Porb = 13.4192d [04627]. Epoch
V0373 Cas    of Min I is given close to the epoch of one of
V0373 Cas    conjunctions. Min II - Min I = 0.58P. Maxima are very
V0373 Cas    sharp. Max - Min II = 0.25P. It is not excluded that the
V0373 Cas    star is an eclipsing one with physical variability of
V0373 Cas    components, but eclipses, if they exist, cause only a very
V0373 Cas    small part of the observed light variations. Range of
V0373 Cas    light variations is given according to [02651]. As a rule
V0373 Cas    the amplitude is close to 0.1m.
V0374 Cas    Min II 12.1.
V0375 Cas    Min II 10.6.
V0377 Cas    VB (A 8.5m; B 9.4m, 2.1", 185deg, 1962).It is not known
V0377 Cas    which component varies. According to [04005] the range
V0377 Cas    of combined brightness variations is 0.26m.
V0377 Cas    According to [07051], const.
V0380 Cas    d = 0.08P.
V0381 Cas    Min II 10.8.
V0388 Cas    Wolf 47 (mu = 0.82", p = 80deg). Faint component of a wide
V0388 Cas    physical pair (p = 294") the bright component of
V0388 Cas    which is the dM2 star Wolf 46 = BD+61deg 195 (9.4).
V0392 Cas    Min II 14.0. P var. Min I = 2429640.390 +
V0392 Cas    4.54094d*E (JD2425300 - 29640); Min I =
V0392 Cas    2429640.390 + 4.54064d*E (JD2429640 - 36900) [04027];
V0392 Cas    since JD2436900 - see Table. Depth of Min var?
V0394 Cas    Min II 15.6.
V0396 Cas    Min II 10.2.
V0399 Cas    Min II 14.1.
V0401 Cas    Min II 15.7.
V0402 Cas    Min II 15.3.
V0406 Cas    Min II 16.8.
V0410 Cas    Bright in 1938 -39. Slow. Not red.
V0423 Cas    Min II 14.3.
V0427 Cas    Min II 13.7.
V0428 Cas    Red.
V0430 Cas    Northern component of a close pair. Red.
V0434 Cas    Red.
V0441 Cas    P = 351.2d?
V0442 Cas    d = 0.025P. P var? Since 1972 P = 3.592120d.
V0444 Cas    Min II 16.0. P var. Min I = 2438651.314 + 2.224808d*E
V0444 Cas    (JD2432850 - 37300); since JD2437300 - see Table. Period
V0444 Cas    variation may be cyclic. Mean elements:
V0444 Cas    Min I = 2443194.258 + 2.224773d*E.
V0445 Cas    Min II 11.08.
V0448 Cas    Min II 15.0.
V0450 Cas    VB A (B 17.5m:, 3.4", 188deg). Range
V0450 Cas    of combined light variations is given.
V0459 Cas    Min II 11.6.
V0466 Cas    In the region of the cluster NGC 457.
V0480 Cas    Min II 14.7.
V0482 Cas    VB A (B 10.0m, F 4 V, 6", 195deg; optical). P = 0.28292d?
V0494 Cas    The chart in [05849] is believed to be distorted.
V0497 Cas    In the region of the cluster IC 1848.
V0498 Cas    In the region of the cluster IC 1848.
V0499 Cas    In the region of the cluster IC 1848.
V0509 Cas    Pulsation of photosphere with P = 3 years.
V0509 Cas    Tenuous shell ejected in 1975 is now falling back to
V0509 Cas    the star.
V0518 Cas    In the region of the cluster Stock 2. Star N136 (Stock 208).
V0520 Cas    Min II 13.1. P var. Min I = 2439069.559 + 0.489832d*E
V0520 Cas    (JD2438580 - 40850); since JD2441150 - see Table.
V0521 Cas    Member of the cluster NGC 7789.
V0523 Cas    Min II 11.34. P var. Min I = 2432054.555 +
V0523 Cas    0.2336882d*E (JD2428545 - 33570) [07008];
V0523 Cas    Min I = 2439029.461 + 0.23368912d*E (JD2439000 - 41300)
V0523 Cas    [07387]; since JD2440480 - see Table.
V0524 Cas    OH, H2O emission. P = 163d?, 191d? 259d?, 620d?
V0526 Cas    Two oscillations are superimposed: P1 = 0.0526d (A1 =
V0526 Cas    0.0036m), P2 = 0.0396d (A2 = 0.0056m); P2/P1 = 0.753.
V0527 Cas    Min II 13.5; Min II - Min I = 0.52P.
V0532 Cas    In the region of the cluster NGC 7789.
V0533 Cas    In the region of the cluster NGC 7789.
V0536 Cas    P var. Max = 2438700.262 + 0.395674d*E
V0536 Cas    (JD2438580 - 39150); Max = 2441186.333 +
V0536 Cas    0.395683D*E (JD2440070 - 41250);
V0536 Cas    since JD2441500 - see Table.
V0540 Cas    Epoch of Max (U) is given.
V0541 Cas    Min II 11.0.
V0542 Cas    In the region of the cluster NGC 7789.
V0544 Cas    Elements given in the Table are valid since JD2428000.
V0546 Cas    In the region of the cluster NGC 103. Min II 14.8.
V0547 Cas    VB A (B 12.4m, M4.5, 2.8", 93deg). Astrometric binary
V0547 Cas    (A = 0.12", P = 15.9a); mu = 1.75", P = 98deg.
V0547 Cas    Variation of combined light is given.
V0551 Cas    P = 45.5d?/57d?/67.5d?.
V0554 Cas    P >= 3500d? D = 400d?
V0559 Cas    VB A (B 7.7m, 0.25", 34deg, 1976). Min II 7.21.
V0566 Cas    VB A (B 8.3m, 1.4", 194deg, 1965).
V0569 Cas    10.0 - 14.7 I.
V0589 Cas    In the cluster NGC 663.
V0592 Cas    White dwarf. Rapid non-periodic fluctuations of brightness
V0592 Cas    on a time scale of several minutes.
V0598 Cas    VB A (B 12m, 19", 0deg). P = 2.825d? [02560].
V0615 Cas    Variable radio source on 10.5 GHz; gamma - and X-ray
V0615 Cas    source?
V0627 Cas    H2O emission.
V0635 Cas    4U 0115 + 634. SB (P = 24.3162d).
V0635 Cas    Pulsar period P = 3.6136s.
V0638 Cas    Epoch of Min is given.
V0742 Cas    SB, Porb = 55.9212d.
V0745 Cas    Component B of the double system observed brighter than in the
V0745 Cas    Hipparcos Input Catalogue.
V0746 Cas    SB, Porb = 27.8d.
V0747 Cas    VB. The variability may be due to the fainter component.
V0961 Cas    The depth of Min II is 0.22.
V0962 Cas    MinII 13.42.
V0971 Cas    The depth of MinII is 0.36.
V0990 Cas    Chomospherically active giant, photometric variations with the rotational period.
V1001 Cas    MinII 14.0.
V1002 Cas    Min II 16.5.
V1006 Cas    Multiperiodic, other periods 0.9249d, 0.7212d.
V1012 Cas    Multiperiodic, other periods 0.3618d:, 0.5195d. VB(A 7.75m, F1V; B 10.39m, G5:V, 0.2", 348deg, 1991).
V1018 Cas    VB (1".5, 200deg, 1976). MinII - MinI = 0.41P.
V1022 Cas    MinII - MinI = 0.67:P.
V1025 Cas    Min II = 12.82.
V1026 Cas    Multiperiodic.
V1027 Cas    Min II = 13.90.
V1030 Cas    Min II = 14.15.
V1031 Cas    Min II = 13.1.
V1032 Cas    Min II = 12.5.
V1036 Cas    VB AB (10.0m + 10.0m, 0.4", 76deg, 1995).
V1037 Cas    Porb = 0.1025d.
V1038 Cas    Min II = 10.05. VB (A 10.7mV; B 11.2mV, 0.7", 314deg, 1991).
V1043 Cas    Min II = 13.5.
V1044 Cas    Min II = 9.63.
V1046 Cas    Min II = 11.7 :.
V1053 Cas    Min II = 15.7.
V1054 Cas    The tabulated amplitude is distorted with GSC 03667-01557.
V1056 Cas    Min II = 14.0 :.
V1060 Cas    Min II = 10.42.
V1061 Cas    Min II = 10.50.
V1062 Cas    Min II = 10.8.
V1063 Cas    Min II = 12.3.
V1064 Cas    Min II = 11.73.
V1065 Cas    Min II = 10.14.
V1066 Cas    Min II = 11.06. MinII - MinI = 0.56P.
V1067 Cas    Min II = 12.9.
V1068 Cas    Min II = 14.78.
V1069 Cas    Min II = 12.72.
V1070 Cas    Min II = 10.47.
V1073 Cas    Outside the tidal radius of the cluster NGC 457.
V1074 Cas    Outside the tidal radius of the cluster NGC 457.
V1075 Cas    Outside the tidal radius of the cluster NGC 457.
V1076 Cas    Min II = 15.97. Outside the tidal radius of the cluster NGC 457.
V1077 Cas    Min II = 15.5. Outside the tidal radius of the cluster NGC 457.
V1079 Cas    Min II = 15.90. Outside the tidal radius of the cluster NGC 457.
V1080 Cas    Min II = 14.5. Outside the tidal radius of the cluster NGC 457.
V1081 Cas    Min II = 17.07. Outside the tidal radius of the cluster NGC 457.
V1082 Cas    Non-member of the cluster NGC 457.
V1083 Cas    Outside the tidal radius of the cluster NGC 457.
V1084 Cas    Min II = 13.8.
V1085 Cas    Non-member of the cluster NGC 457.
V1087 Cas    Non-member of the cluster NGC 457.
V1088 Cas    Outside the tidal radius of the cluster NGC 457.
V1090 Cas    Min II = 16.5. Non-member of the cluster NGC 457.
V1092 Cas    Outside the tidal radius of the cluster NGC 457.
V1093 Cas    Min II = 14.8. Non-member of the cluster NGC 457.
V1094 Cas    Min II = 12.35 :.
V1095 Cas    Outside the tidal radius of the cluster NGC 457.
V1096 Cas    Min II = 15.2. Outside the tidal radius of the cluster NGC 457.
V1097 Cas    Outside the tidal radius of the cluster NGC 457.
V1098 Cas    Min II = 16.8 :.
V1099 Cas    Outside the tidal radius of the cluster NGC 457.
V1101 Cas    Min II = 16.6. Outside the tidal radius of the cluster NGC 457.
V1102 Cas    Outside the tidal radius of the cluster NGC 457.
V1103 Cas    Min II = 11.95 :. MinII - MinI = 0.531P.
V1104 Cas    Outside the tidal radius of the cluster NGC 457.
V1105 Cas    Outside the tidal radius of the cluster NGC 457.
V1106 Cas    Min II = 13.05.
V1107 Cas    Min II = 13.5.
V1110 Cas    Min II = 10.7 :. MinII - MinI = 0.710P.
V1112 Cas    A twice longer period with minima of the same depth is possible.
V1114 Cas    Min II = 19.0.
V1115 Cas    Min II = 14.2.
V1120 Cas    Min II = 17.2.
V1121 Cas    Min II = 18.45 :.
V1122 Cas    VB B (A = NSV 00542, 7.3m; B 14", 143deg, 2007; 3 more components).
V1123 Cas    Amplitude(Min II)=  0.11mag. MinII - MinI = 0.73P.
V1125 Cas    Min II = 17.65.
V1131 Cas    Min II = 12.54.
V1133 Cas    Min II = 13.62 :.
V1134 Cas    Min II = 19.34.
V1135 Cas    Min II = 18.85.
V1136 Cas    Min II = 16.77.
V1137 Cas    Min II = 12.28.
V1138 Cas    Min II = 13.4.
V1139 Cas    Amplitude(Min II)=  0.30mag.
V1141 Cas    Min II = 12.76. MinII - MinI = 0.44P.
V1142 Cas    Min II = 11.15.
V1155 Cas    VB A (A 11.1mV; B 13.2mV, 7", 219deg, 2000).
V1156 Cas    VB A (B 14.0mV, 12", 222deg, 2000).
V1159 Cas    Min II = 11.91.
V1160 Cas    Min II = 12.0. A twice shorter period is possible.
V1162 Cas    Min II = 11.67. MinII - MinI = 0.230P.
V1164 Cas    Min II = 12.27 :.
V1166 Cas    Min II = 11.80.
V1170 Cas    Min II = 11.47.
V1172 Cas    Min II = 12.8.
V1174 Cas    Min II = 12.85.
V1175 Cas    Min II = 10.22 :.
V1176 Cas    Min II = 11.7 :. MinII - MinI = 0.494P.
V1177 Cas    Min II = 11.47 :. MinII - MinI = 0.53P.
V1178 Cas    Min II = 12.92.
V1179 Cas    Min II = 13.0. VB A (B 13.8mV, 29", 323deg, 1999). The tabulated magnitudes can be distorted by the companion.
V1183 Cas    Multiperiodic.
V1194 Cas    Multiperiodic.
V1236 Cas    O'Connell effect.
alf   Cas    VB A (B 14.5m, 17.6", 272deg; C 13.5m, 38", 105deg;
alf   Cas    D 8.5m, 64.4", 280deg.)
bet   Cas    VB A (B 13.7m, 31.3", 243deg); SB (P = 27d).
bet   Cas    [Fe/H] = 0.64.
gam   Cas    VB A (B 11.0m, 2.2", 248deg; C 13.0m, 52.2", 348deg).
gam   Cas    In HII region S 185. X-ray source MX 0053 + 60.
gam   Cas    v sin i = 310 km/s.
del   Cas    VB A (B 11.5m, 31.7", 66deg). Min II 2.75. Min II - Min I =
del   Cas    361d. The elements given in the Table are still not
del   Cas    confirmed by anyone.
iot   Cas    VB A (B 6.89m, 2.3", 239deg; C 8.40m, 7.2", 114deg).
iot   Cas    Astrometric binary (a = 0.113", P = 52.4a). Max (V) - Max
iot   Cas    (lambda 1550) = 0.4P; A (lambda 1550) = 0.40m. The range
iot   Cas    of total brightness variation of components A and
iot   Cas    B is given.
kap   Cas    P = 0.09028d, P(Vr) = 0.14035d [02588]; P = 7d [08876].
omi   Cas    VB A (B 11.7m, 33.6", 303deg). SB1 (P = 1033d);
omi   Cas    V sin I = 220 km/s.
pi.   Cas    SB, Porb = 1.9642d.
rho   Cas    Usually varies within the limits 4.4m - 5.2m V.
rho   Cas    In November 1945 the peculiar decrease of brightness began
rho   Cas    lasting for 165d and in September 1946 the star reached
rho   Cas    the middle of the deepest minimum (JD2432070) lasting for
rho   Cas    320d. Then the brightness began to increase symmetrically
rho   Cas    and by July 1947 the star attained its normal brightness
rho   Cas    [00957]. Photographic magnitudes varied in the limits
rho   Cas    5.4m - 8.3m. Spectrum description [08878].
B     Cas    Tycho Brahe's supernova. Stellar object is not identified
B     Cas    optically up to now.
R     Cen    VB A (B 12m, 28", 218deg). Epoch
R     Cen    of Min I is given. Min I 0.00P, Max I 0.23P, Min II
R     Cen    0.47P, Max II 0.64P. Max I 5.8, Max II 6.0,
R     Cen    Min I 11.1, Min II 8.3. P var. P = 561.3d
R     Cen    before 1918; since 1918 - see Table. H2O maser.
V     Cen    In the field of the open cluster NGC 5662.
Z     Cen    SN 1895 (NGC 5253).
RR    Cen    Min II 7.63. dII = 0.08P. P var. Min I = 2424231.0910 +
RR    Cen    0.60568807d*E + 2.31d*10**(-10)*E**2 (JD2414170 -
RR    Cen    33470) [00006]. Current elements - see Table.
RS    Cen    A 1118-61?
RT    Cen    P var.
RZ    Cen    Min II 9.4.
SS    Cen    Min II 9.5.
ST    Cen    Min II 11.30, DII = 0.22P. Max II (before
ST    Cen    Min I) 10.65.
SU    Cen    Min II 9.2.
SV    Cen    Min II 9.45. Delta(m) var. P var. Min = 2433053.358 +
SV    Cen    1.6594795d*E - 7.61d*10**(-8)*E**2 (JD2412608 - 42097).
SV    Cen    Cyclic (32a - 33.6a) period variations were noted in
SV    Cen    [00009, 05212]. Since 1978 - see Table. P Cyg profiles in
SV    Cen    the spectrum.
SX    Cen    For mean light Max = 2426835 + 615d*E.
SY    Cen    d = 0.05P.
SZ    Cen    VB. Min II 8.7.
TX    Cen    VB? B - V: +1.39, +2.11.
TZ    Cen    The co-ordinates in the Table are based on [00015].
TZ    Cen    According to [00016], no star brighter than 14m was found
TZ    Cen    in this position. The co-ordinates in [00015] may be in
TZ    Cen    error.
UW    Cen    IR excess.In Max varies semiregularly, P ~42d [08832].
UZ    Cen    VB A (B 13.8m, 4", 191deg). Max II = 2440746.2 +
UZ    Cen    2.35529d*E.
VW    Cen    VB A (B ~15m?, ~8", ~180deg). B - V: +1.01, +1.71.
VW    Cen    [A/H] = 0.3.
VZ    Cen    Min II 8.4.
WX    Cen    B - V ~ +0.45, U - B ~ -0.72.
WX    Cen    Proposed as an optical counterpart of the transient X-ray
WX    Cen    source Cen X-2 [05314], though no optical bursts were
WX    Cen    observed.
WZ    Cen    Min II 14.2.
ZZ    Cen    VB C (A 9.4m, B9; B 10.8m, 8", 314deg; C = ZZ Cen,
ZZ    Cen    9", 259deg; D = AA Cen, 9", 110deg).
AA    Cen    VB D (see ZZ Cen).
AB    Cen    d = 0.05P.
AP    Cen    Epoch of Min is given.
AS    Cen    Min II 13.2.
AV    Cen    Min II 14.1.
AZ    Cen    The shape of the light curve varies.
BD    Cen    Min II 10.7.
BF    Cen    In the field of the open cluster NGC 3766. Min II 8.8.
BG    Cen    Min II 12.3.
BH    Cen    In the open cluster IC 2994. Min II 11.1 V.
BI    Cen    Delta(S) = 2.
BK    Cen    P2 = 2.236d, A1 = 0.54m, A2 = 0.22m [08835].
BV    Cen    The mean cycle between outbursts <= 149.4d [07301]. The
BV    Cen    tabulated elements correspond to Max of the eclipsing
BV    Cen    light curve, phi (Min) = 0.25P. The range of the eclipsing
BV    Cen    variability is 12.8 - 13.3.
CN    Cen    Min II 13.3.
DI    Cen    Min II 12.3, Min II - Min I = 0.494P, DII = 0.08P:.
DT    Cen    Red.
DX    Cen    The P star in a pair.
DY    Cen    All spectral lines are very weak. No IR excess. The
DY    Cen    photometric behaviour outside major Min is described in
DY    Cen    [08836].
EP    Cen    Min II 11.5.
EU    Cen    The P star in a pair.
GI    Cen    In the field of the globular cluster NGC 5286.
GM    Cen    The chart in [06286] is wrong.
IQ    Cen    d = 0.04P.
IW    Cen    Min II 12.1.
IX    Cen    In the field of the open cluster NGC 3706.
IY    Cen    In the field of the open cluster IC 2944.
IZ    Cen    B - V = 1.7.
KK    Cen    B - V: +1.08, +1.62.
KM    Cen    Min II 13.3.
KN    Cen    B - V: +1.36, +1.75. [A/H] = 0.2.
KQ    Cen    Alternating periods 136d, 159d.
KT    Cen    B - V: +0.46. Min II 12.72. Min II - Min I = 0.392P
KT    Cen    (JD2441686 - 721); apsidal motion is observed [08094].
KY    Cen    Min II 13.3.
KZ    Cen    B - V: +0.30, +0.72.
LL    Cen    Min II 13.1.
LR    Cen    Min II 12.30.
LT    Cen    Min II 9.6.
LU    Cen    The period may be twice longer.
LV    Cen    B - V: +1.3, +1.7.
LW    Cen    Min II 9.6. In the field of the open cluster IC 2944.
LX    Cen    Min II 13.55.
LZ    Cen    Min II 8.50.
MM    Cen    Min II 12.7.
MN    Cen    Min II 8.7. VB A (B 10.9m, 7", 147deg).
MP    Cen    Min II 10.0.
MQ    Cen    Min II 10.1.
MR    Cen    Min II 10.5.
MV    Cen    Min II 14.6.
MY    Cen    B - V: +1.58, +1.94.
NO    Cen    Min II 14.2.
NP    Cen    Min II 10.2.
NY    Cen    Min II 11.9.
OO    Cen    B - V = 1.84.
OP    Cen    Min II 13.8.
OU    Cen    Min II 10.9.
OV    Cen    Min II 11.0.
OX    Cen    Min II 14.3.
QS    Cen    d = 0.03P.
QT    Cen    Min II 13.4.
QY    Cen    B - V = 2.16.
QZ    Cen    P var? The shape of the light curve varies?
V0339 Cen    VB A (B ~13m, SP). B - V: +1.08, +1.47.
V0343 Cen    Min II 13.5.
V0344 Cen    Min II 12.3.
V0346 Cen    In the field of the open cluster Stock 14. Min II 8.8.
V0346 Cen    Min II = 2421966.835 + 6.32189d*E.
V0348 Cen    d = 0.010P.
V0349 Cen    Min II 14.5.
V0350 Cen    Min II 10.3. Min II = 2430870.192 + 3.216906d*E.
V0351 Cen    Epoch of Min is given.
V0356 Cen    Min II 15.0.
V0358 Cen    Epoch of Min is given.
V0365 Cen    d = 0.040P.
V0373 Cen    VB A (B ~4" np).
V0377 Cen    d = 0.003P.
V0379 Cen    Min II 8.9.
V0380 Cen    Min II 10.0.
V0383 Cen    Min II 13.6:, Min II - Min I = 0.609P.
V0384 Cen    Min II 12.2. DII = 0.062P. Min II - Min I = 0.667P.
V0385 Cen    Min II 13.0.
V0388 Cen    Min II 15.7.
V0399 Cen    d = 0.020P. Min II 13.1.
V0405 Cen    P var, 30d - 40d.
V0412 Cen    VB A (B 59", 266deg).
V0419 Cen    P var. Max = 2428099.25 + 5.50713d*E (JD2428099 - 33573);
V0419 Cen    since JD2434900 - see Table.
V0420 Cen    B - V: +0.45, +0.97. P var. Nonlinear term:
V0420 Cen    -0.000090d*E**2.
V0427 Cen    Epoch of Min is given.
V0436 Cen    SB (P = 0.0669d). Photometric P during supermaxima
V0436 Cen    0.06383d [08838]. Rapid oscillations in supermaxima
V0436 Cen    Delta(m) ~0.002m, P ~19.6s [08049].
V0440 Cen    d = 0.033P. Min II is possible.
V0443 Cen    d = 0.025P.
V0491 Cen    Very flat minima; close companion?
V0495 Cen    d = 0.042P. Min II 10.6. Min II - Min I = 0.520P.
V0496 Cen    Possible member of the open cluster NGC 4755.
V0496 Cen    B - V: +1.02, +1.33.
V0498 Cen    P may be twice shorter.
V0499 Cen    (k - b)2 = 0.23.
V0504 Cen    Semiregular  variations (P1 ~130d, P2 ~411d)
V0504 Cen    are also observed [08836].
V0506 Cen    The chart in [06286] is wrong.
V0508 Cen    Min II 13.2.
V0526 Cen    Delta(m) var. P var. Max = 2425707.540 + 0.56153d*E
V0526 Cen    (1929 - 1930); during 1931 - 1940 - see Table.
V0527 Cen    The chart in [06286] is wrong.
V0532 Cen    Star 1 [09078]. X-ray source 3A 1431-409.
V0544 Cen    2AS E 1440-39? [05962]. The chart in [06286] is wrong.
V0545 Cen    Magnitude in Max var (12.6 - 14.5), P = 1800d?
V0553 Cen    [Fe/H] = -0.1; [C/Fe] = +0.8.
V0565 Cen    Min II 13.9. Type RR is not excluded (P = 0.238072d).
V0574 Cen    sp star of a pair.
V0577 Cen    Min II 14.4.
V0585 Cen    Min II 13.0.
V0592 Cen    Mean brightness var.
V0593 Cen    Possible member of the open cluster Stock 16. Min II 11.2.
V0594 Cen    V133 (omega Cen); non-member of the cluster. Min II 14.4.
V0606 Cen    Min II 9.8.
V0607 Cen    Min II 14.1.
V0608 Cen    Min II 13.1.
V0609 Cen    Min II 13.6.
V0615 Cen    Min II 14.0.
V0617 Cen    Min II 13.8:.
V0619 Cen    In the field of the open cluster NGC 5316.
V0621 Cen    d = 0.05P.
V0624 Cen    Min II 14.9.
V0625 Cen    Min II 15.0.
V0627 Cen    d = 0.02P.
V0628 Cen    Min II 13.2.
V0630 Cen    Min II 14.2. d = 0.06P.
V0635 Cen    Min II 13.9.
V0636 Cen    Min II 8.8.
V0644 Cen    During the faint phase in 1951 the shell spectrum was
V0644 Cen    observed [02128]. Type E with a very long period is
V0644 Cen    possible [06763].
V0645 Cen    Proxima Cen = alpha Cen C. mu = 3.809", P = 281.7deg.
V0645 Cen    Soft X-ray source.
V0646 Cen    d = 0.022P. Min II 9.1.
V0662 Cen    P ~2.48d or 2.95d.
V0672 Cen    Min II 11.4 - 11.6 (var).
V0673 Cen    Depth of Min II 0.05m.
V0674 Cen    Blazhko effect: Pi = 29.5d. 0.15P <= M - m <= 0.23P.
V0676 Cen    Min II 12.5.
V0677 Cen    Min II 11.6.
V0678 Cen    Min II 10.6.
V0679 Cen    9.8"p, 1.1"n from CPD -62deg 2167.
V0679 Cen    The star is at the edge of a dark cloud in a bright nebula,
V0679 Cen    a part of IC 2944, in the field of a very poor open
V0679 Cen    cluster. Since 1950 till 1954 faded by 2.5m. Rather red.
V0679 Cen    "Screening" by the edge of a dark nebula?
V0682 Cen    IR excess.
V0684 Cen    Depth of Min II 0.05m.
V0685 Cen    Min II 9.5.
V0686 Cen    RV type is not excluded.
V0687 Cen    Min II 14.1. DII = 0.12P. Min II - Min I = 0.580P.
V0688 Cen    Min II 12.7.
V0689 Cen    Min II 12.1.
V0690 Cen    Depth of Min II 0.03m.
V0692 Cen    Min II 11.6. Min II - Min I = 0.481P.
V0701 Cen    VB? d = 0.026P. Min II 9.1.
V0704 Cen    IR excess.
V0716 Cen    Min II 6.21.
V0742 Cen    Min II 10.1.
V0743 Cen    (k - b)2 = 0.20. Elements almost as well satisfactory:
V0743 Cen    Max = 2439243.6465 + 0.10222560d*E.
V0745 Cen    Min II 9.6.
V0746 Cen    = V467 Cen. Marked as V467 Cen in the chart.
V0747 Cen    Min II 10.05.
V0748 Cen    B - V: +0.31, +1.21; U - B: -0.66, -0.21. d = 0.106P.
V0748 Cen    Narrow Halpha emission. Outside eclipses shows variations
V0748 Cen    by 0.05m - 0.1m during several days or several weeks
V0748 Cen    (probably irregularly) [06968].
V0752 Cen    Min II 9.61. dI = dII = 0.047P.
V0753 Cen    (k - b)2 = 0.20. In the field of the open cluster NGC 3960;
V0753 Cen    probably non-member. Type DSCT is possible.
V0754 Cen    Slight Min II.
V0755 Cen    In the Coalsack.
V0756 Cen    In the Coalsack. High excitation lines (OVII, OVIII, CV)
V0756 Cen    are present in the spectrum. WR type is possible [07372].
V0757 Cen    Min II 8.6.
V0758 Cen    d = 0.07P. Min II 9.15.
V0759 Cen    Min II 7.56.
V0761 Cen    IR excess.
V0763 Cen    VB A (B 13m, 7", 163deg).
V0766 Cen    VB A (B 10.01m, B0Ibp, 9", 318deg). IR excess.
V0767 Cen    VB A (B 11.52m, 21", 350deg).
V0768 Cen    Possible P: 60d - 80d.
V0770 Cen    According to [07570], const?
V0772 Cen    In the region of the open cluster IC 2944.
V0775 Cen    EB type is possible. Deep Min II.
V0777 Cen    Deep Min II.
V0779 Cen    Cen X-3 (3U 1118-60). B - V: +1.04; U - B:  -0.08.
V0779 Cen    Min II 13.39. Porb var. The shape of the light curve
V0779 Cen    varies. Epoch of Min I is given. Epochs of Min II coincide
V0779 Cen    with the moments of X-ray eclipses. X-ray pulses are
V0779 Cen    observed with Ppuls = 4.834477s (epoch JD2442785.3);
V0779 Cen    Ppuls decreases [07612]. No rapid optical oscillations
V0779 Cen    were found.
V0783 Cen    B - V: +0.35.
V0784 Cen    Very red.
V0788 Cen    Min II 5.90.
V0790 Cen    VB B (A 4.52m; 60", 343deg).
V0791 Cen    In the region of globular cluster omega Cen (NGC 5139).
V0791 Cen    Cluster non-member.
V0795 Cen    VB A (B 12.29m, 33.9", 170deg; C 12.79m, 36", 220deg).
V0801 Cen    4U 1145 - 61 = 2S 1145 - 619. Primary component has a low
V0801 Cen    density envelope expanding with the velocity of 1800 km/s.
V0801 Cen    V sin i = 290 km/s. X-ray pulsar (P = 291.8s
V0801 Cen    [08883]). Max (X) = 2442519.5 + 187.5d*E [08881].
V0803 Cen    Extremely hot hydrogen-deficient helium star.
V0807 Cen    VB (9.9m, 10.1m, 0.4", 258deg, 1931).
V0807 Cen    It is not known which of the components varies.
V0810 Cen    Member of the cluster Stock 14.
V0813 Cen    In the region of globular cluster omega Cen (NGC 5139).
V0813 Cen    V65 (NGC 5139).
V0814 Cen    In the region of globular cluster omega Cen (NGC 5139).
V0814 Cen    V78 (NGC 5139). Min II 14.165:. Primary
V0814 Cen    component is probably intrinsically variable [08884].
V0816 Cen    Primary oscillation is superimposed by the oscillations
V0816 Cen    with freguencies: F2 = 4.9229, F3 = 4.7343, F4 = 4.9317
V0816 Cen    [02591].
V0820 Cen    [Fe/H] = -2.5; Vr = +260 km/s.
V0822 Cen    Cen X-4.
V0825 Cen    In the region of globular cluster omega Cen (NGC 5139).
V0825 Cen    Cluster non-member. V2 (NGC 5139).
V0826 Cen    In the region of globular cluster omega Cen (NGC 5139).
V0826 Cen    Cluster non-member. V129 (NGC 5139).
V0902 Cen    VB, rho = 12". Variability may be spurious.
V0915 Cen    The variability type is not quite consistent with the spectral
V0915 Cen    type (B9II/III).
V0921 Cen    High proper motion (LTT 4397) not confirmed by HIPPARCOS data.
V0933 Cen    HIPPARCOS data contradict the luminosity class V.
V1015 Cen    Variability type and luminosity class (III) do not agree.
V1045 Cen    Background field star.
V1048 Cen    P2 = 0.743241 d. P1 is in the table. P2/P1 = 0.8058.
V1053 Cen    MinII 12.57.
V1054 Cen    MinII 12.18:.
V1057 Cen    MinII 12.7.
V1059 Cen    VB A (B 12.7R, 25" p).
V1061 Cen    MinII 9.61.
V1086 Cen    Observations influenced by a 12.2m companion in 35" to north.
V1087 Cen    Apsidal motion, U = 169 years [126]. VB AB (9.6m, 10.3m, 0.8", 27deg, 1937).
V1089 Cen    MinII - MinI = 0.57P.
V1094 Cen    O'Connell effect [100].
V1095 Cen    VB A (B 12.9m, 18", 172deg, 1999).
V1100 Cen    VB A (B 13.2m, 17", 257deg, 2000; C 15.5m, 11", 129deg, 1999).
V1104 Cen    VB (A 10.2m; B 12.0m, 13", 76deg, 2000). According to [236], a double-periodicity eclipsing star: EB, P1 = 0.876114d and EA, P2 = 19.11d (MinI 2451938.733 [100]).
V1119 Cen    VB (A 9.4m; B 12.6m, 2.8", 123deg, 1929).
V1129 Cen    EB-type variations (Max 9.55m) with brightenings to 9.1m, lasting for 40 days, each 357 days. No close bright infrared companion. HeII emission in the spectrum.
V1133 Cen    VB (A 9.5m; B 11.5m, 0.7", 271deg, 1927).
V1142 Cen    MinII - MinI = 0.40P. DII = 0.11P.
V1155 Cen    X-ray source. VB B (A = HR 4940, 4.69m, B5V; B 11", 79deg, 2001; C 9.16mKs, 1.6", 268deg, 2000).
V1166 Cen    MinII - MinI = 0.41P.
V1176 Cen    MinII - MinI = 0.59P.
V1180 Cen    VB A (B 12.7m, 12", 270deg, 1997).
V1182 Cen    Blend (B 13.6mpg, 25", 277deg; C 13.9mpg, 18", 32deg, 1998; several components at larger separations). Tabulated variability limits are distorted by the companions.
V1185 Cen    VB A (B 14.6m, 7", 198deg, 1997).
V1194 Cen    VB (A 10.02m; B 10.5m, 12", 309deg, 1999).
V1197 Cen    VB A (B 13.6mV, 15", 211deg; C 14.1mV, 14", 307deg; D 10.3mJ, 5", 337deg, 2000; etc.).
V1198 Cen    MinII - MinI = 0.48P.
V1202 Cen    VB A (B 11.6m, 7", 356deg, 1991).
V1210 Cen    The tabulated period is for the fundamental mode, P1 = 3.037d.
V1214 Cen    Min II = 10.69. The tabulated elements are for the eclipses. Pulsations: P = 0.121252d, with an amplitude of 0.04m.
V1215 Cen    VB A (A 11.87mR; B 13.11mR, 17", 51deg, 1999).
V1216 Cen    A twice longer period is also possible.
V1218 Cen    Min II = 13.5.
V1219 Cen    Min II = 10.65.
V1229 Cen    Min II = 9.49. P varies. dP/dt = +1.67 x 10^(-5) d/yr. VB AB (A 10.29m; B 10.44m, 0.4", 231deg, 1991; C 10.80m, AB-C 16", 324deg, 2000). AB varies; combined ABC magnitudes are tabulated.
V1237 Cen    Min II = 11.7.
V1238 Cen    VB B (A = V1239 Cen; AB 6", 276deg, 2000).
V1239 Cen    VB A (B = V1238 Cen, 6", 276deg, 2000).
V1242 Cen    Min II = 13.8.
V1254 Cen    Min II = 11.75.
V1258 Cen    The tabulated light elements are for eclipses in quiescence. The range of orbital variations is 15.4m - 17.0m in outburst, 18.2m - 22.2m in quiescence.
V1259 Cen    Multiperiodic.
V1260 Cen    Min II = 9.50.
V1261 Cen    VB B (A 4.23mV; AB 25", 100deg, 2007).
V1262 Cen    Min II = 12.6.
V1263 Cen    Min II = 12.5.
V1264 Cen    Min II = 12.50. The tabulated light elements are for eclipses. The DSCT period is 0.0734d, with an amplitude of 0.21m.
V1265 Cen    Tabulated is a period twice shorter than that suggested in [138]. Also detected is P = 3.537421d, close to the tabulated one but differing from it.
V1266 Cen    Min II = 8.13. VB A (AaAb speckle: Aa 8.10m, Ab 11.00m, 0.1", 76deg, 2008; B 10.84m, 9", 283deg, 2000).
V1269 Cen    Min II = 13.5.
V1284 Cen    Min II = 13.35.
V1286 Cen    Min II = 11.55.
V1289 Cen    Min II = 11.1.
V1294 Cen    Min II = 8.07.
V1296 Cen    Min II = 11.34.
V1298 Cen    Min II = 15.15.
V1312 Cen    Min II = 16.85:.
V1313 Cen    Min II = 18.00.
V1314 Cen    Min II = 13.55.
V1315 Cen    Min II = 16.6.
V1316 Cen    Min II = 13.80.
V1317 Cen    Min II = 15.6 :.
V1318 Cen    Min II = 14.25.
V1320 Cen    Min II = 18.40.
V1321 Cen    Min II = 17.10.
V1322 Cen    Min II = 15.19:.
V1326 Cen    Min II = 11.67.
V1347 Cen    Min II = 11.1.
V1351 Cen    Min II = 11.27.
V1356 Cen    Min II = 12.96.
V1358 Cen    VB A (B 13m, 15", 34deg, 2000).
V1362 Cen    P varies, dP/dt = +0.19 x 10^{-5} d/yr. VB AB (9.6mm 12.1m, 0.8", 243deg, 1945).
bet   Cen    VB A (B 4.1m, 1.3", 251deg, 1960). SB1 (P = 352d
bet   Cen    [08887]. Multiperiodicity; sometimes brightness is constant
bet   Cen    [08215]. Soft X-ray source.
del   Cen    VB A (B 4.8m, 68.6", 325deg; C 6.5m, 16.6", 227deg).
eps   Cen    VB A (B 13.0m, 36.0", 158deg). There is a secondary light
eps   Cen    oscillation with the amplitude of 0.0034m and elements:
eps   Cen    Max = 2441041.058 + 0.17696d*E.
eta   Cen    VB A (B 13.5m, 5.6", 270deg, 1897); SB?
mu.   Cen    VB A (B 13.63m, 48", 128deg).
omi 1 Cen    VB A (B 11.4m, 13.5", 125deg).
T     Cep    P var. Max = 2414252 + 386.05d*E (JD2406900 - 20490);
T     Cep    Max = 2431086 + 394.93d*E (JD2420490 - 32900);
T     Cep    Max = 2440262 + 379.22d*E (JD2432900 - 42200); since
T     Cep    JD2442200 Max = 2444171 + 392.7d*E. Mean value of the
T     Cep    period is given in the Table. SiO maser.
U     Cep    VB A (B 11.83m, 13.9", 62deg; C 12.3m, 23.0", 318deg).
U     Cep    0.010P <= d <= 0.040P. Min II 6.93. P var. Min I =
U     Cep    2407890.3346 + 2.4928551d*E + 5.15d*10**(-9)*E**2
U     Cep    (JD2388855 - 2440790) [06468]; analysis of period
U     Cep    variations in this interval see also in [07395];
U     Cep    Min I = 2441395.3604 + 2.4931048d*E (JD2440790 - 41600);
U     Cep    Min I = 2441679.5716 + 2.4930432d*E (JD2441600 - 950);
U     Cep    Min I = 2443753.7982 + 2.4930679d*E (JD2442100 - 43800);
U     Cep    since JD2444000 - see Table. Shape of the light curve
U     Cep    and depth of minima vary. Brightness of the secondary (G8)
U     Cep    varies sporadically. Subgiant brightening accompanies
U     Cep    eruptive mass transfer. The gaseous stream moving to the
U     Cep    primary (B7) component forms around it gaseous ring or
U     Cep    disc [08889].
W     Cep    Slow oscillations with Pi ~2000d are superimposed by
W     Cep    oscillations with P ~350d.
X     Cep    OH emission?
RS    Cep    d = 0.039P. P var. Min = 2417140.469 + 12.419925d*E
RS    Cep    (JD2410000 - 31000) [02431]; since JD2431000 - see Table.
RZ    Cep    P var. Max = 2411640.654 + 0.308697d*E
RZ    Cep    (JD2411640 - 15000); Max = 2417144.620 + 0.3086203d*E
RZ    Cep    (JD2415600 - 20200); Max = 2421175.611 +
RZ    Cep    0.3086699d*E (JD2421175 - 23000); Max =
RZ    Cep    2423768.475 + 0.3086918d*E (JD2423000 - 31700);
RZ    Cep    Max = 2433768.493 + 0.3086383d*E (JD2433700 -
RZ    Cep    38300) [08890]; Max = 2438207.938 + 0.308645d*E
RZ    Cep    (JD2438200 - 39040) [03879]; Max = 2440834.579 +
RZ    Cep    0.3086735d*E (JD2440800 - 42640) [08890];
RZ    Cep    since JD2442640 - see Table. Shape of the light curve and
RZ    Cep    the amplitude A vary with the Blazhko effect period
RZ    Cep    Pb = 96.8*P0 = 29.88d; Min A = 2441464.147 + 29.88d*N
RZ    Cep    [08891]. Long period variation of P0 with a period ~50
RZ    Cep    years is possible. Delta(S) = 6.
SS    Cep    Mean brightness varies with cycles from some hundreds to
SS    Cep    thousands days.
SU    Cep    Min II 10.6.
SV    Cep    IR excess.
SX    Cep    In the region of the nebula NGC 7023.
SY    Cep    Min II 12.70. P var?
SZ    Cep    VB A (B 12.3m, 24.9", 263deg). S4/6e.
TT    Cep    VB A (B 17.0m, 8", 160deg).
TY    Cep    Epoch of Min I is given.
UZ    Cep    P var. Max = 2440969 + 297.68d*E (JD2414000 - 42000);
UZ    Cep    since JD2440000 - see Table.
VV    Cep    VB (0.05", 174deg, 1950)? 0.066P <= D <= 0.091P;
VV    Cep    0.040P <= d <= 0.077P. Depth of eclipses: 2.30m (lambda
VV    Cep    3500 A), 1.9m (U), 0.4m (B). M-component is of SRC type:
VV    Cep    Max = 2443045 + 118.37d*E [08698, 08894]; A(V) <= 0.33m.
VV    Cep    Light oscillations are also noted with P ~58d [08895],
VV    Cep    25d and 150d [08896]. B-component may be also an intrinsic
VV    Cep    variable [02416]. Gaseous streams. Strong variable magnetic
VV    Cep    field.
VW    Cep    VB A (B 10.3m, a = 0.51", P = 30.45a [08897]); mu alpha =
VW    Cep    +0.0899s, mu delta = +0.560". Min II 7.56.
VW    Cep    Shape of the light curve and depths of Min I and Min II
VW    Cep    vary. P var. Min I = 2433483.4257 + 0.27831758d*E +
VW    Cep    0.050d*cos(0.004813deg*(E - 4700)) (JD2424763 - 41200)
VW    Cep    [06483]; since JD2441000 - see Table. Period
VW    Cep    change study see also in [08899]. X-ray source.
VZ    Cep    Min II 9.93.
WX    Cep    Min II 9.14; dI = 0.01P, dII = 0.00P.
WY    Cep    Min II 11.5. P var [02545].
WZ    Cep    Min II 11.9.
XX    Cep    Min II 9.24 V. P var. Min I = 2425096.449 + 2.337340d*E
XX    Cep    (JD2414930 - 30000); Min I = 2441539.4917 + 2.3373059d*E
XX    Cep    (JD2430000 - 42300) [08902]. Since JD2441500 - see Table.
XY    Cep    Min II 10.10. P var?
XZ    Cep    Min II 8.43.
ZZ    Cep    VB A (B 10.2m, A2 P, 3.6", 202deg; C 10.87m, A5V,
ZZ    Cep    20.6", 219deg). Min II 8.74.
AH    Cep    Min II 7.03. Depth of minima varies. P var.
AH    Cep    Min I = 2434989.3702 + 1.7747274d*E (JD2415500 - 35000)
AH    Cep    [03604]; since  JD2434900 - see Table: +3.12d*10**(-9)*E**2.
AI    Cep    Min II 9.48.
AN    Cep    Since JD2425200 primary and secondary maxima and minima
AN    Cep    appeared, and mean cycle became 254d.
AV    Cep    d <= 0.04P.
BB    Cep    d = 0.050P.
BE    Cep    Min II 13.0.
BF    Cep    P var. Max = 2437236 + 426.11d*E (JD2423600 - 37300);
BF    Cep    Max = 2441665 + 442.3d*E (JD2437300 - 42500); since
BF    Cep    JD2442500 - see Table.
BH    Cep    Sometimes strong Algol-like light weakenings are observed.
BO    Cep    Sometimes strong Algol-like light weakenings are observed.
CO    Cep    Min II 12.6; Min II - Min I = 0.552P; DII = 0.080P.
CP    Cep    P var?
CQ    Cep    Shape of the light curve and depth of minima vary.
CQ    Cep    According to [07401] on 1969 March 28/29 on the phase
CQ    Cep    0.56P a light decrease by 0.1m was observed and then a
CQ    Cep    rapid flare by 0.35m U, 0.13m B, 0.14m V. P var. Nonlinear
CQ    Cep    term: -10**(-9)*E**2.
CR    Cep    P var. Max = 2436846.94 + 6.23318d*E (JD2415000 - 30000)
CR    Cep    [03157]; since JD2430000 - see Table.
CV    Cep    S7/1.5. Mean brightness varies with a cycle ~2000d [00159].
CW    Cep    VB A (B 12.29m, 20", 310deg). Min II 8.01;
CW    Cep    Min II -  Min I = 0.478P (1972 yr). There is a sinusoidal
CW    Cep    term in the elements: +0.0250d*sin(0.0626deg*E - 28.3deg).
CW    Cep    Apsidal motion with P = 43a.
CX    Cep    Min II 12.16.
DD    Cep    P var. Max = 2427960 + 167.6d*E (JD2427900 - 30000);
DD    Cep    Max = 2429968 + 173.0d*E (JD2429900 - 33600);
DD    Cep    since JD2433600 - see Table.
DH    Cep    In the region of the cluster NGC 7380. Apsidal motion with
DH    Cep    P = 2.6a [00165].
DK    Cep    Min II 12.4.
DL    Cep    Min II 12.7.
DO    Cep    VB B (A 9.87m, M4V; a = 2,4", P = 44.78a, e = 0.408);
DO    Cep    mu = 0.852", P = 242.6deg.
DP    Cep    Min II 14.4.
DQ    Cep    Multiperiodicity: P0 = 0.12420d: [08137], P1 = 0.061177d
DQ    Cep    [08914].
DX    Cep    P var. Max = 2430603.712 + 0.5260395d*E (JD2415700 - 31000)
DX    Cep    [00001]; since JD2431000 - see Table. Delta(S) = 7.
DY    Cep    Min II 11.8.
EE    Cep    A var?
EF    Cep    Min II 12.6. P var?
EG    Cep    Min II 9.61. P var. Min I = 2439774.3322 + 0.54462091d*E
EG    Cep    (JD2415200 - 41000) [00001]; since JD2441000 - see Table.
EH    Cep    In the dark cloud near the diffuse nebula and the cluster
EH    Cep    NGC 7023.
EI    Cep    Min II 7.98.
EK    Cep    Min II 8.06; Min II - Min I = 0.545P (1965). Min II =
EK    Cep    2439022.8484 + 4.427797d*E [08160].
EK    Cep    Apsidal motion (P = 4700a  +- 600a) [08923].
EL    Cep    P var.
EM    Cep    In the region of the cluster NGC 7160. VB A (a 12.8m,
EM    Cep    19.8", 281deg; B 7.9m, 62.5", 146deg). Min II 7.16.
EM    Cep    Shape of the light curve and depth of minima vary.
EO    Cep    Min II 12.3.
EP    Cep    In the cluster NGC 188. Min II 17.0.
EQ    Cep    In the cluster NGC 188. Min II 16.7.
ER    Cep    In the cluster NGC 188. Min II 16.27.
ES    Cep    In the cluster NGC 188. Min II 15.8.
ES    Cep    P var. Min I = 2439082.238 + 0.34468d*E (JD2438480 - 39090);
ES    Cep    Min I = 2439236.501 + 0.34264d*E (JD2439090 - 39280);
ES    Cep    Min I = 2439594.548 + 0.34250d*E (JD2439400 - 39600);
ES    Cep    since JD2439600 - see Table. A var.
EX    Cep    Min II 11.6.
EY    Cep    Min II 10.4.
EZ    Cep    P var. Max = 2416803.627 + 0.378990d*E (JD2415400 - 20000)
EZ    Cep    [00001]; since JD2420000 - see Table.
FH    Cep    Min II 12.1.
FL    Cep    d = 0.02P.
FS    Cep    Min II 12.0.
FT    Cep    VB A (B 18.3m, 5", 27deg). In the region of the diffuse
FT    Cep    nebula and the cluster NGC 7023.
FU    Cep    In the region of the diffuse nebula and the cluster
FU    Cep    NGC 7023.
FV    Cep    In the region of the diffuse nebula and the cluster
FV    Cep    NGC 7023. P = 0.4628d.
FW    Cep    In the region of the diffuse nebula and the cluster
FW    Cep    NGC 7023.
GI    Cep    Min II 11.9.
GK    Cep    Min II 7.35; dI = dII = 0.03P; Min II - Min I = 0.502P.
GK    Cep    P var. Min I = 2425189.526 + 0.9361614d*E
GK    Cep    (JD2415000 - 27500); Min I = 2438694.7070 + 0.9361714d*E
GK    Cep    (JD2427500 - 38200) [00001]; since JD2438200 - see Table.
GL    Cep    In the region of the diffuse nebula IC 1396 and the
GL    Cep    cluster Tr 37.
GM    Cep    In the region of the diffuse nebula IC 1396 and the
GM    Cep    cluster Tr 37.
GP    Cep    In the region of the HII zone S 132. Quadruple system,
GP    Cep    consisting of a WN6 + O8-B0III: eclipsing pair
GP    Cep    (P = 6.6883d) physically associated with an O + O pair
GP    Cep    (P = 3.4698d); the latter pair may be also an eclipsing
GP    Cep    or ellipsoidal variable [08931].
GS    Cep    Min II 10.6.
GT    Cep    Min II 8.6.
GW    Cep    Min II 12.00.
HK    Cep    Min II 14.4.
HZ    Cep    In the region of the diffuse nebula and the cluster
HZ    Cep    NGC 7023.
IL    Cep    VB A (B 11.91m, 7", 326deg); P = 2.802d?
IM    Cep    Min II 13.6.
IO    Cep    Min II 11.7.
IP    Cep    Min II 12.1.
IR    Cep    VB (Delta(m) ~0.0m, 0.0" -0.2"). P var.
IR    Cep    Max = 2431060.878 + 2.114016d*E (JD2428335 - 31060) [00001];
IR    Cep    since JD2440900 - see Table.
IV    Cep    VB B (A 16m; B 2.1", 191deg).
IW    Cep    Min II 13.7; Min II - Min I = 0.52P.
IX    Cep    d = 0.03P. Min II 17.0.
KL    Cep    d = 0.019P.
KP    Cep    Depth of Min II 0.03m.
KV    Cep    Min II 14.3.
KY    Cep    Flare with 65 sec duration. There is a blue object on the
KY    Cep    place of the flare [00001].
KZ    Cep    VB (8.6m, 8.6m; 1.9", 348deg). Depths of spectral lines
KZ    Cep    vary: P = 0.212938d [06488].
LL    Cep    Min II 14.0.
LM    Cep    Min II 12.8.
LP    Cep    Min II 13.8; Min II - Min I = 0.55P.
LQ    Cep    Eastern component of a double star.
LU    Cep    VB.
LW    Cep    Depth of Min II 0.05m.
LZ    Cep    Min II 5.63. In the Table: P(Vr) [04627].
MN    Cep    Depth of Min II 0.08m?
MQ    Cep    Min II 15.7.
MT    Cep    Min II 15.5.
MX    Cep    SB (P = 16.03d) [08947].
MY    Cep    In the cluster NGC 7419. Emission OH, H2O.
MZ    Cep    In the region of the cluster NGC 7419.
NN    Cep    Min II 8.52.
NR    Cep    Min II 13.6; d = 0.025P?
NS    Cep    Depth of Min II 0.04m.
NW    Cep    Preceding component of a close VB. Min II 10.7.
NY    Cep    VB A (B 10.33m, 10", 190deg); d = 0.003P; SB2, e = 0.49;
NY    Cep    Delta(gamma) = gamma2 - gamma1 = 32 km/s  [07412].
OS    Cep    Very red.
OT    Cep    Min II 13.3.
OZ    Cep    Red.
PS    Cep    In the region of the cluster NGC 7380. SB2 (P = 2.09168d)
PS    Cep    [05479].
PV    Cep    In the dark cloud near the diffuse nebula and the cluster
PV    Cep    NGC 7023. At the apex of the bright variable fan nebula.
PW    Cep    In the region of the diffuse nebular and the cluster
PW    Cep    NGC 7023.
QZ    Cep    The map of surroundings given in [04015] for BV 323 is in
QZ    Cep    reality the map for BV 324 = QZ Cep. Min II 11.9.
V0338 Cep    Min II 9.52.
V0342 Cep    B - V = +3.6.
V0344 Cep    B - V = +4.4.
V0345 Cep    B - V = +5.0.
V0346 Cep    B - V = +4.6.
V0347 Cep    B - V = +4.5.
V0351 Cep    VB A (B 13m, 20", 135deg). P var. Max = 2430615.57 +
V0351 Cep    2.80511d*E (JD2429160 - 34300); Max = 2435749.12 +
V0351 Cep    12.80556d*E (JD2435310 - 40885) [02830]. Since
V0351 Cep    JD2442020 - see Table.
V0421 Cep    SB, Porb1 = 5.4136d, Porb2 = 225.44d.
V0447 Cep    The variability may be due to the fainter (B) component.
V0448 Cep    SB, Porb = 7.7320d.
V0453 Cep    SB, Porb = 54.723d.
V0454 Cep    SB, Porb = 5.6556d.
V0711 Cep    Variability refers to combined brightness of two nearly equal
V0711 Cep    components at 5" separation.
V0727 Cep    MinII 14.48.
V0732 Cep    Amplitude and mean brightness strongly vary.
V0737 Cep    Though originally suspected as a "missing" star BD+62 1936 (which is probably GSC 4252.00433), an identification with a preceding star (probably GSC 4252.00821) was immediately suggested
V0738 Cep    VB A (B 14.1V, 14", 132deg, 2000).
V0741 Cep    VB (9.2mHp, 12.7mHp, 0.7", 9deg, 1991).
V0743 Cep    MinII - MinI = 0.53P:. SB2.
V0747 Cep    Min II = 10.05. MinII - MinI = 0.25P.
V0748 Cep    Min II = 13.3.
V0749 Cep    Min II = 10.9.
V0750 Cep    Min II = 11.63 :. MinII - MinI = 0.44:P.
V0751 Cep    Min II = 13.7.
V0752 Cep    Min II = 13.4.
V0753 Cep    Min II = 11.45.
V0754 Cep    Min II = 12.25.
V0755 Cep    Min II = 12.95.
V0756 Cep    Min II = 14.20.
V0757 Cep    Min II = 14.7.
V0758 Cep    Min II = 13.5.
V0759 Cep    Probable non-member of the cluster NGC 188.
V0760 Cep    Min II = 15.15. Non-member of the cluster NGC 188.
V0761 Cep    Non-member of the cluster NGC 188.
V0764 Cep    Min II = 17.86. Non-member of the cluster NGC 188.
V0767 Cep    Min II = 15.34.
V0775 Cep    Min II = 14.05.
V0777 Cep    Min II = 16.56.
V0782 Cep    Min II = 15.58.
V0784 Cep    Amplitude(Min II)=  0.07mag.
V0785 Cep    Min II = 14.52.
V0789 Cep    Min II = 14.80. O'Connell effect. Non-member of the cluster NGC 188.
V0790 Cep    Min II = 12.80. Non-member of the cluster NGC 188.
V0791 Cep    Min II = 17.19. Non-member of the cluster NGC 188.
V0792 Cep    Non-member of the cluster NGC 188.
V0793 Cep    Min II = 16.31. Non-member of the cluster NGC 188.
V0794 Cep    Multiperiodic.
V0796 Cep    Min II = 12.85.
V0797 Cep    Min II = 14.95.
V0798 Cep    Min II = 12.43. MinII - MinI = 0.232P.
V0800 Cep    Min II = 13.7.
V0801 Cep    Min II = 13.1 :.
V0802 Cep    Min II = 13.65.
V0803 Cep    Min II = 14.2.
V0804 Cep    Min II = 13.45.
V0805 Cep    Min II = 12.46.
V0806 Cep    Min II = 11.34.
V0808 Cep    Min II = 11.78 :.
V0810 Cep    O'Connell effect.
V0818 Cep    Cluster non-member.
V0821 Cep    VB A (B 17.9mR, 4", 253deg, 2000).
V0822 Cep    Type EW with a twice longer period is not excluded [001].
V0835 Cep    Type RRC with the light elements Max = 2451511.899 + 0.2261d x E is not excluded.
V0839 Cep    VB AB (9.9m, 11.7m, 0.2", 212deg, 2008). MinII - MinI = 0.511P.
V0850 Cep    MinII - MinI = 0.599:P.
V0873 Cep    Multiperiodic.
V0874 Cep    Multiperiodic.
V0880 Cep    MinII - MinI = 0.540P.
V0881 Cep    MinII - MinI = 0.476:P.
V0882 Cep    VB A (B 14.6m, 7", 274deg, 1999).
V0897 Cep    MinII - MinI = 0.518P.
V0898 Cep    MinII - MinI = 0.670P.
V0919 Cep    MinII - MinI = 0.44P.
V0921 Cep    MinII - MinI = 0.429P.
V0922 Cep    MinII - MinI = 0.585P. VB A (A 10.6mJ; B 11.9mJ, 11", 44deg; C 13.6mJ, 4", 76deg, 1999). Tabulated magnitudes are influenced with the companions.
V0944 Cep    MinII - MinI = 0.528P.
V0954 Cep    O'Connell effect.
V0957 Cep    MinII - MinI = 0.560P.
V0961 Cep    MinII-MinI=0.482P.
bet   Cep    VB A (A 6m, 0.204", 47.2deg, 1977.9; B 7.84m, A2V, 13.6",
bet   Cep    250deg). SB1 (Porb = 10.893d) [06486]. P var.
bet   Cep    Max(Vr) = 2417359.715 + 0.1904795d*E (JD2415750 - 22000);
bet   Cep    Max(Vr) = 2422203.790 + 0.1904844d*E +
bet   Cep    2.9440d*10**(-11)*E**2 + 3.2671d*10**(-17)*E**3
bet   Cep    (JD2422000 - 42630) [00177]. Elements given in the Table
bet   Cep    satisfy observations in 1967 - 69.
del   Cep    VB A (B 13.0m, 20.0", 285deg; C 6.10m - 6.37m, B7IV,
del   Cep    41.0", 191deg. P var. Max = 2393659.856 + 5.366438d*E
del   Cep    (JD2372200 - 96900); Max = 2413960.73 + 5.366386d*E
del   Cep    (JD2396900 - 2414050); since JD2414050 - see Table.
del   Cep    All observations in the interval JD2373090 - 45000 are
del   Cep    well represented also by the elements with a square term:
del   Cep    Max = 2442756.490 + 5.366270d*E - 7d*6*10**(-9)*E**2
del   Cep    [08632].
eps   Cep    VB A (B 9.5m, 127.8", 15deg, 1918).
eps   Cep    Multiperiodicity: P2 = 0.068073d
eps   Cep    (A2/2 = 0.0061m), P3 = 0.011823d? (A3/2 = 0.0022m);
eps   Cep    A1/2 = 0.0079m.
zet   Cep    Radial velocity varies.
mu.   Cep    VB A (B 12.3m, 19.4", 262deg; C 12.7m, 41", 299deg).
mu.   Cep    There is also the cycle with 4400d duration [08957].
W     Cet    S5.5/2e.
RR    Cet    [Fe/H] = -1.26. P var. During JD2417500 - 28820
RR    Cet    Max = 2417501.444 + 0.55302577d*E; since JD2433180 - see
RR    Cet    Table. According to [08726], the graph of O - C deviations
RR    Cet    from the elements given in [03506] is approximately
RR    Cet    sinusoidal, with Pi = 2600d and the amplitude 0.025d.
RU    Cet    (k - b)2 = 0.01. Delta(m) var? P var [02455]. Max =
RU    Cet    2426964.019 + 0.5863003d*E (JD2426500 - 28430)
RU    Cet    [00181]; Max = 2434143.056 + 0.5862676d*E
RU    Cet    (JD2433100 - 35820) [02431]; since JD2435820 - see Table.
RV    Cet    Delta(S) = 9.
RW    Cet    Min II 10.5. P var. During JD2426500 - 41000
RW    Cet    Max = 2426585.503 + 0.9751814d*E [00001]; since
RW    Cet    JD2441000 - see Table.
RX    Cet    Delta(S) = 5. P var. Before JD2428500 Max =
RX    Cet    2425938.271 + 0.5737100d*E [03506]; since
RX    Cet    JD2430000 - see Table.
RZ    Cet    Delta(S) = 6.7. P var. During JD2426585 - 28630
RZ    Cet    Max = 2426585.448 + 0.510633d*E [03506]; current
RZ    Cet    elements - see Table.
SS    Cet    d = 0.025P. P var. Min = 2429321.250 + 2.9739509d*E
SS    Cet    (JD2427340 - 30700) [02419]; Min = 2430698.160 +
SS    Cet    2.973992d*E (JD2429300 - 36650) [03115];
SS    Cet    since JD2440000 - see Table.
SV    Cet    Min II 14.9.
TT    Cet    Min II 11.1.
TU    Cet    D = 0.043P. Min II 10.9. Min II - Min I = 0.478P.
TU    Cet    According to [03564], the spectrum is K2.
TV    Cet    Min II 9.10. DII = 0.03P. Min II - Min I = 0.494P.
TW    Cet    Min II 11.14. P var. Min I = 2430965.595 +
TW    Cet    0.316852d*E (JD2427650 - 31000) [00192]; Min I =
TW    Cet    2433611.3121 + 0.316846d*E (JD2433530 - 615)
TW    Cet    [00001]; since JD2440000 - see Table.
TX    Cet    B - V: +0.34, +0.37. Min II 11.12.
TY    Cet    Min II 12.1.
UU    Cet    (k - b)2 = 0.08. P var. Blazhko effect?
UV    Cet    VB B (A 12.45m, dM5.5e; a = 2.1", P = 25a).
VV    Cet    Min II 11.0. EB type is also possible. RR type with twice
VV    Cet    shorter period is not excluded.
VX    Cet    d = 0.026P.
VY    Cet    Min II 11.70.
VZ    Cet    ADS 1778 B (B 0.61", 122deg; A = omicron Cet).
VZ    Cet    Small variations are also observed on the time scale of
VZ    Cet    several hours, with superimposed 10 - 15 minute variations
VZ    Cet    and rare flares of approximately 2 minute duration
VZ    Cet    [06492]. A possible white dwarf with an accretion
VZ    Cet    disc [08926].
WW    Cet    VR var (P = 0.160d) [04712].
WW    Cet    Rapid oscillations (~10 min) of brightness are observed
WW    Cet    [04709].
WZ    Cet    Min II 11.0.
XY    Cet    d = 0.02P. Min II 9.34.
YY    Cet    Min II 9.2.
ZZ    Cet    4 stable oscillations are observed simultaneously:
ZZ    Cet    P1 = 213.132605s, P2 = 212.768427s, P3 = 274.250814s,
ZZ    Cet    P4 = 274.774562s.
AA    Cet    ADS 1581 A (B 7.7m vis, SB 2, F5, 8.5", 304deg).
AA    Cet    Min II 6.7:. dII = 0.065P.
AB    Cet    ADS 1849 A (B 9.30m, 12", 293deg). SB? (VR var,
AB    Cet    P = 2.997814d). The period of magnetic variations is
AB    Cet    15.9d [08932].
AD    Cet    ADS 180 A (B 10m, 3", 4deg).
CL    Cet    Type ELL: is also possible.
EE    Cet    The variability may be due to the fainter (B) component.
EL    Cet    SB2.
EV    Cet    The depth of MinII is 0.44.
FH    Cet    MinII 13.8.
FL    Cet    The light elements given are for the eclipses.
FR    Cet    A shell star of the spectral type A.
FU    Cet    Chomospherically active giant, photometric variations with the rotational period.
GO    Cet    Variable brown dwarf.
GP    Cet    Min II = 9.89.
GR    Cet    Min II = 11.47. P varies. dP/dt = -0.39x10^(-5) d/yr.
GW    Cet    Blazhko effect with a possible period about 84d.
GY    Cet    Pulsation periods: 595s, 335s, etc. Porb = 81.54min.
GZ    Cet    Porb = 0.060d.
HI    Cet    Min II = 13.07.
HK    Cet    Multiperiodic. VB A (B Sp L6, 0".3).
HS    Cet    Min II = 11.1.
del   Cet    Nonlinear term: +2.20d*10**(-11)*E**2.
omi   Cet    ADS 1778 A (B = VZ Cet, 0.61", 122deg). Maser
omi   Cet    SiO, OH, H2O.
S     Cha    VB A (B 9.29m, 23", 134deg).
T     Cha    Occasionally quasiperiodic light changes are observed with
T     Cha    periods 3.2323d, 3.4375d, 4.1800d, 3.2436d operating
T     Cha    during 6 - 26 cycles. IR excess.
Z     Cha    VB A (B 5.6"). Eclipses: Min =
Z     Cha    2440264.68232 + 0.0744992195d*E + 7.88d*10**(-13)*E**2
Z     Cha    [08938]. D = 0.065P; d = 0.026P. Depth of Min:
Z     Cha    1.73m - 2.11m B before the eclipse; 1.38m - 1.97m B after
Z     Cha    the eclipse. Periodic variations during Min light [07000].
Z     Cha    Variations with P = 27.7s during a supermaximum [08049].
RS    Cha    EA/DM. Min II 6.53. One of the components is a pulsating
RS    Cha    variable of DSCT type. P is in the range from 0.074d
RS    Cha    to 0.097d [08403]. Delta(M) = 0.01m - 0.03m in the combined
RS    Cha    light.
RW    Cha    Min II 14.6.
RY    Cha    Min II 14.0.
RZ    Cha    Min II 8.8. DII = 0.11P.
SY    Cha    Quasiperiodic variations were observed. (P = 6.2d [04305],
SY    Cha    P = 7.6d [08946]).
TW    Cha    Quasiperiodic variations (P = 8.68d [04462]).
VW    Cha    IR excess.
VZ    Cha    Quasiperiodic variations (P = 7.27d).
YZ    Cha    Delta(m) (Min II) = 0.4m.
CG    Cha    Min II 14.4.
CH    Cha    Min II 15.1.
CX    Cha    Min II 15.5. Uncertain elements.
CY    Cha    Min II 14.0.
CZ    Cha    Min II 14.6.
DD    Cha    Min II 14.7.
DG    Cha    Min II 14.5.
ES    Cha    In the eta Cha cluster.
ET    Cha    In the eta Cha cluster.
FO    Cha    VB A (B 10.75m, 12", 161deg, 2000).
GM    Cha    VB B (A 10.25m; AB 10", 57deg, 2000).
GO    Cha    Min II = 10.95. dP/dt = -0.20 x 10^(-5) d/yr.
GP    Cha    P2 = 1190d.
GQ    Cha    Min II = 13.8.
GS    Cha    VB A (B 14.21m, 5", 326deg, 2000).
GT    Cha    VB A (B 14.52m, 8", 319deg, 2000).
HK    Cha    VB? (0.2").
HM    Cha    VB B (A 9.09m; AB 10", 295deg, 2000).
HN    Cha    VB B (A = VW Cha, 6.96m; AB 17", 221deg, 2000).
HO    Cha    VB B (A = NSV 18675, 6.83m; AB 16", 82deg, 2000).
HP    Cha    VB AB (2.7", 1986). Combined magnitudes are tabulated.
IT    Cha    Min II = 13.1.
zet   Cha    SB.
S     Cir    Min II 10.9.
T     Cir    Min II 9.4.
U     Cir    P var. Before JD2417000 Max = 2412560 + 151d*E.
V     Cir    Min II 11.0. According to [00210], varies in the range
V     Cir    10.8m - 13.0m pg.
W     Cir    Found in Lupus, in 4deg to the north from the position
W     Cir    published by the discoverer [00211].
TW    Cir    Min II 13.3.
UY    Cir    Red.
UZ    Cir    Epoch of main Max is given. Resembles R Cen.
UZ    Cir    Max I - Max II = 160d.
VX    Cir    P var. Before JD2418000 Max = 2414360 + 427d*E.
AQ    Cir    Possibly EW type with twice longer period.
AR    Cir    The magnitude in Min light possibly corresponds to an
AR    Cir    unresolved companion.
AT    Cir    d = 0.02d:.
AX    Cir    SB. VB? (6.5m; 6.5m; 0.5", 143deg, 1913).
BD    Cir    Min II 9.5.
BF    Cir    Min II 8.9.
BG    Cir    Min II 10.3.
BN    Cir    Deep Min II. Twice shorter period is not excluded.
BR    Cir    Cir X-1. According to [08951], the object does not coincide
BR    Cir    with the star (B = 22.5m) labelled as L in the chart in
BR    Cir    [02911] but is situated in ~1" to the south of it and has
BR    Cir    M > 23.5m on IIIa-J plates. Gradual increase of X-ray
BR    Cir    intensity is periodically stopped by an abrupt intensity
BR    Cir    fall. The moments of such transitions T are represented by
BR    Cir    the elements T = 2443292.118 + 16.595d*E [02926]. The X-ray
BR    Cir    intensity falls are accompanied by IR and radio bursts.
BR    Cir    Vr (e alpha) = +250 km/s. In 25' from the supernova
BR    Cir    remnant G 321.9-0.3.
DK    Cir    MinII - MinI = 0.75P.
EL    Cir    VB A (B 11.50m, 17", 119deg, 2000).
tet   Cir    VB (6.2m, 6.2m, 0.1", 96deg).
T     Col    SiO maser.
U     Col    Min II 10.5.
Y     Col    V2 (NGC 1851).
Z     Col    V1 (NGC 1851).
RS    Col    Min II 9.97. dII = 0.021P.
RY    Col    (k - b)2 = 0.10. P var; nonlinear term: -3.38*10**(9)E**2.
RZ    Col    Min II 11.20.
TV    Col    2A 0526 - 328. VB A (B 15.79m, 10", 330deg). Epoch of Max
TV    Col    of short-term photometric variations is given. The
TV    Col    following elements describe, respectively, moments of Max
TV    Col    Vr for Balmer lines and moments of Max for the
TV    Col    comparatively long-term photometric variations which are
TV    Col    due to the beat phenomenon for the photometric and
TV    Col    spectral periods: Max Vr = 2444227.631 + 0.228600d*E;
TV    Col    Max = 2444191.5 + 4.024d*E. Flickering up to 0.15m B and
TV    Col    flares up to 0.3m U are also observed [08960].
VW    Col    Variability may be due to component B.
AW    Col    MinII - MinI = 0.79P.
AY    Col    Min II = 10.63.
AZ    Col    Min II = 11.65. P varies. dP/dt = -0.17x10^(-5) d/yr.
BC    Col    Min II = 13.5.
BD    Col    VB B (A = NSV 16739, 4.4m; AB 34", 110deg, 1999).
BE    Col    Min II = 11.55.
R     Com    OH emission.
S     Com    Delta(S) = 8.
T     Com    OH, H2O emission.
U     Com    Delta(S) = 5.
V     Com    P var. Max = 2424518.219 + 0.46913844d*E
V     Com    (JD2420900 - 26900) [00218]; since JD2438100 - see Table.
V     Com    Delta(S) = 8.
W     Com    Radio source ON 231.
X     Com    Z = 0.092. Spectrum description [07415, 08966].
Y     Com    In the region of the globular cluster M 53 (NGC 5024).
Z     Com    In the region of the globular cluster M 53 (NGC 5024).
RR    Com    In the region of the globular cluster M 53 (NGC 5024).
RS    Com    In the region of the globular cluster NGC 5053.
RT    Com    In the region of the globular cluster NGC 5053. A var;
RT    Com    P var. Max = 2423113.496 + 0.5651925d*E (JD2422700 -
RT    Com    26450) [00222]; since JD2438535 - see Table.
RU    Com    In the region of the globular cluster M 53 (NGC 5024).
RV    Com    In the region of the globular cluster M 53 (NGC 5024).
RW    Com    In the region of the Comae Berenices cluster. dI = 0.04P;
RW    Com    Min II 11.56. P var.
RW    Com    Min I = 2433040.406 + 0.23734705d*E (JD2419680 - 34550)
RW    Com    [00185]; since JD2439600 - see Table.
RY    Com    P var. Max = 2425007.450 + 0.46894835d*E (JD2425000 -
RY    Com    27500) [03506]; Max = 2432674.390 + 0.4689397d*E
RY    Com    (JD2432600 - 38110) [03415]; since JD2438100 - see Table.
RY    Com    (k - b)2 = 0.07.
RZ    Com    Possible member of the Comae Berenices cluster. Min II
RZ    Com    11.09; dI = 0.043P, dII = 0.039P. P var.
RZ    Com    Min I = 2433396.737 + 0.33850556d*E (JD2425000 - 33300)
RZ    Com    [00226]; since JD2433300 - see Table.
RZ    Com    Shape of the light curve varies.
SS    Com    Min II 11.9.
ST    Com    Delta(S) = 10.
SX    Com    In the region of the globular cluster NGC 4147.
SZ    Com    In the region of the globular cluster NGC 4147.
TU    Com    Shape of the light curve, A and P vary. Mean elements
TU    Com    are given in the Table. Possible period of Blazhko effect
TU    Com    is 75d [03584]. [Fe/H] = -1.43.
UU    Com    Member of the Comae Berenices cluster. Light variations
UU    Com    are due to rotation and pulsations of the star. Rotational
UU    Com    period is 2.1953d or 1.0256d or 0.9178d. Period of
UU    Com    pulsations is 0.0227d (A ~0.01m). According to [07985]
UU    Com    there are two periods of pulsations: P1 = 0.0274d and
UU    Com    P2 = 0.0209d
UU    Com    (P2/P1 = 0.76).
UV    Com    [Fe/H] = -1.44.
UW    Com    [Fe/H] = -1.22.
UX    Com    Min II 10.13. P var; nonlinear term: -3.75d*10**(-8)*E**2.
UY    Com    [Fe/H] = -1.51.
UZ    Com    [Fe/H] = -1.44.
VV    Com    [Fe/H] = -1.53.
VW    Com    VB (12.00m, dM 3.5e; 12.3m, dM 4e, 3.0", 23deg, 1945).
VW    Com    Range of total brightness variation
VW    Com    is given. According to [08363] the component B is
VW    Com    variable. However both components may be variables.
VY    Com    Min II 14.5.
AI    Com    Member of the Comae Berenices cluster. VB A (B 6.63m,
AI    Com    145", 251deg). Pulsations are possible: P = 0.052d
AI    Com    (A = 0.02m) [08975].
AL    Com    Within 8' to the south-east from the nucleus of M 88
AL    Com    (NGC 4501) galaxy.
AQ    Com    Min II 15.7.
BM    Com    Min II 13.8.
BS    Com    P var. Max = 2434453.31 + 0.36341d*E (JD2434130 - 35230);
BS    Com    since JD2435590 - see Table. Shape of the light curve
BS    Com    varies.
BZ    Com    [Fe/H] = -1.21.
CC    Com    In the region of the Comae Berenices cluster. Min II
CC    Com    12.09; dI = 0.03P.
CD    Com    [Fe/H] = -1.78.
CF    Com    Shape of the light curve varies.
CG    Com    [Fe/H] = -1.06.
CI    Com    RRC?
CK    Com    P var. Max = 2437370.71 + 0.6940159d*E (JD2437370 - 40130);
CK    Com    Max = 2441630.35 + 0.6939080d*E (JD2440130 - 41630);
CK    Com    since JD2441630 - see Table. Blazhko effect.
CK    Com    [Fe/H] = -1.68.
CL    Com    [Fe/H] = -1.00.
CN    Com    Min II 13.5.
CP    Com    [Fe/H] = -1.19.
CT    Com    In the region of the Comae Berenices cluster.
CV    Com    In the region of the Comae Berenices cluster.
CX    Com    In the region of the Comae Berenices cluster. Not member
CX    Com    of the cluster.
DD    Com    Min II 14.90.
DG    Com    Min II 14.6.
DL    Com    P var?
DR    Com    EW? P = 0.45184d?
DS    Com    [Fe/H] = -1.32.
DT    Com    [Fe/H] = -1.60.
DU    Com    [Fe/H] = -1.45.
DV    Com    [Fe/H] = -1.57.
DW    Com    [Fe/H] = -1.53.
EE    Com    P = 0.539533d also satisfies observations. [Fe/H] = -1.64.
EF    Com    [Fe/H] = -1.90.
EG    Com    [Fe/H] = -1.29.
EI    Com    [Fe/H] = -1.68.
EL    Com    P = 0.52362d also satisfies observations.
EM    Com    [Fe/H] = -1.64.
EN    Com    [Fe/H] = -1.19.
EO    Com    [Fe/H] = -1.51.
EP    Com    [Fe/H] = -0.98.
EQ    Com    Min II 15.3.
ER    Com    [Fe/H] = -1.51.
ES    Com    [Fe/H] = -2.02.
EW    Com    [Fe/H] = -1.77.
EX    Com    P = 0.558359d? [Fe/H] = -1.48.
EY    Com    Min II 18.0.
EZ    Com    P = 0.568349d? [Fe/H] = -1.16.
FG    Com    P = 0.3098d also satisfies observations.
FK    Com    Wide emission lines, Halpha and H, K CaII, of variable
FK    Com    intensity. Epoch of light minimum is given.
FM    Com    The member of the Comae Berenices cluster. Multiperiodicity.
FM    Com    Cycle of 0.0713d was observed also [08989].
FO    Com    In the region of the Comae Berenices cluster.
FP    Com    In the region of the Comae Berenices cluster. mu = 0.23",
FP    Com    P = 158deg. Red.
FZ    Com    P = 4.704864d?
GM    Com    In the region of the Comae Berenices cluster.
GN    Com    Member of the Comae Berenices cluster. P > 1d.
GO    Com    In the region of the Comae Berenices cluster.
GP    Com    mu = 0.38", p = 286deg. SB (Porb = 0.032306d).
GP    Com    Unique object G 61-29. Consists of two interacting white
GP    Com    dwarfs. The lower mass star, a helium white dwarf,
GP    Com    transfers mass to the higher mass star surrounded by an
GP    Com    accretion disk. Usually flares are being observed with an
GP    Com    amplitude about 0.2m V, 0.5m U lasting about 20 seconds
GP    Com    [07417, 08991]. Sometimes periods of photometric activity
GP    Com    arise when amplitude of light variations reaches 0.6m V
GP    Com    and sharp passages from maxima to minima are being
GP    Com    observed; the duration of these minima reaches up to 0.14d
GP    Com    [07417]. When the star is most active, periodic light
GP    Com    oscillations appear with P = 105 seconds and amplitude
GP    Com    0.05m - 0.10m V [07062].
GQ    Com    Z = 0.165. Emission H, [OIII]. Irregular light variations.
GQ    Com    B - V = +0.16.
GT    Com    Minor planet (679) Pax.
HH    Com    Epoch of Min in V system is given.
HI    Com    In the region of the Comae Berenices cluster.
HK    Com    In the region of the Comae Berenices cluster.
HM    Com    In the region of the Comae Berenices cluster.
HN    Com    In the region of the Comae Berenices cluster.
HO    Com    In the region of the Comae Berenices cluster.
HP    Com    In the region of the Comae Berenices cluster.
HQ    Com    In the region of the Comae Berenices cluster.
HR    Com    In the region of the Comae Berenices cluster.
HS    Com    In the region of the Comae Berenices cluster.
HT    Com    In the region of the Comae Berenices cluster.
HU    Com    In the region of the Comae Berenices cluster.
HV    Com    In the region of the Comae Berenices cluster.
HW    Com    In the region of the Comae Berenices cluster.
MM    Com    MinII 12.80.
MN    Com    Variable brown dwarf.
MR    Com    MinII 12.43.
MT    Com    Small-amplitude pulsations with characteristic periods 1344, 1236, 668 seconds.
MW    Com    Min II = 10.5.
MX    Com    Min II = 11.94.
MZ    Com    Min II = 10.2 :.
NN    Com    Min II = 12.67.
NS    Com    Min II = 13.5.
NV    Com    Min II = 12.15.
NW    Com    Multiperiodic, with several periods in the DSCTC range (one of them tabulated) and several GDOR periods (P = 0.42779d and others).
OP    Com    Multiperiodic? Blazhko effect?
OR    Com    P varies [001]. Blazhko effect? [026].
OW    Com    Min II = 16.3.
OX    Com    Min II = 16.1 :.
R     CrA    In the head of the bright cometary nebula NGC 6729.
R     CrA    IR excess.
S     CrA    VB A (B 13.5m, 1", 137deg). IR excess.
T     CrA    In the bright cometary nebula NGC 6729. IR excess.
V     CrA    Quasiperiodic variations (P ~75d, Delta(V) ~ 0.2m - 0.9m).
V     CrA    IR excess.
RS    CrA    sp of two close stars; each of them or both may be
RS    CrA    identified with CoD -39deg 13082.
RW    CrA    Min II 9.4.
SS    CrA    V1 (NGC 6541).
SV    CrA    The period may be twice shorter.
TY    CrA    VB A (B 13.3m, 4", 138deg; C 58", 24deg).
TY    CrA    In the bright nebula NGC 6726/27. P = 1.92d is not
TY    CrA    excluded, in that case Min II = Min I. On the basis of
TY    CrA    visual observations 8.7 - 12.4 v (presumably "spurious
TY    CrA    variability" due to the difficulties of estimates over
TY    CrA    the bright background of the nebula), and the star
TY    CrA    was classified as INSA.
TZ    CrA    Min II 9.72.
UU    CrA    Min II 11.0.
UX    CrA    The period may be twice shorter.
UY    CrA    P var?
VV    CrA    In the region of the bright nebula NGC 6729. IR excess.
AF    CrA    P var. Before JD2418060 Max = 2413710 + 483d*E; since
AF    CrA    JD2418060 - see Table.
AL    CrA    B - V: +0.65, +1.30. [A/H] = -0.2.
AN    CrA    P var. Nonlinear term: -0.006d*10**(-6)*E**2.
AU    CrA    P var. Nonlinear term: -0.026d*10**(-6)*E**2.
AY    CrA    Min II 15.2.
BG    CrA    Min II 15.1.
BH    CrA    P var. Nonlinear term: -0.023d*10**(-6)*E**2.
CM    CrA    P var. Nonlinear term: -0.007d*10**(-6)*E**2.
CR    CrA    Min II 15.7.
CS    CrA    Min II 15.2.
CY    CrA    P var. Nonlinear term: -0.002d*10**(-6)*E**2.
DG    CrA    In the region of the bright nebula NGC 6729. IR excess.
DL    CrA    Min II 13.6.
DN    CrA    P var. Nonlinear term: +0.006d*10**(-6)*E**2.
DZ    CrA    d = 0.02P.
EE    CrA    mpg var, 13.5m - 15.5m, P2 = 3000d - 5000d
EE    CrA    Delta(m) (P1 = 167d) ~1.5m.
EK    CrA    P var. Before JD2422600 Max = 2411870 + 421d*E.
FF    CrA    Before JD2423000 Max = 2411530 + 140.2d*E.
FK    CrA    Min II 14.5.
FS    CrA    Min II 14.5.
FW    CrA    Before JD2416600 Max = 2411190 + 112.2d*E.
GS    CrA    Before JD2422600 Max = 2414070 + 284d*E.
IT    CrA    Min II 13.6.
KM    CrA    The chart in [06286] is wrong.
KQ    CrA    [A/H] = -0.7. B - V: +0.76, +1.23.
KT    CrA    Red.
LU    CrA    P = 182d is possible.
MS    CrA    Yellow.
MT    CrA    Min II 13.1.
NO    CrA    Reddish.
QR    CrA    Reddish.
V0347 CrA    B - V: +0.82, +1.17.
V0350 CrA    Min II 13.4.
V0385 CrA    The period may be spurious.
V0413 CrA    (k - b)2 = 0.11.
V0428 CrA    The period may be twice shorter.
V0449 CrA    [A/H] = -0.3.
V0454 CrA    Min II 10.5.
V0455 CrA    d = 0.05P. Min II 13.7.
V0457 CrA    Epoch of Min is given. EW type is also possible, in that
V0457 CrA    case the value of P should be doubled.
V0465 CrA    Min II 14.2.
V0467 CrA    P var?
V0471 CrA    Min II 13.3.
V0478 CrA    Sometimes a cycle 60d - 70d.
V0480 CrA    Min II 13.9.
V0490 CrA    P var? The elements represent the observations of 1944.
V0493 CrA    P var?
V0501 CrA    Min II 13.4. Twice shorter period is possible.
V0503 CrA    d = 0.03P.
V0511 CrA    Twice longer period is possible.
V0512 CrA    P var?
V0513 CrA    Min II 13.2.
V0514 CrA    Min II 14.0.
V0527 CrA    P var.
V0535 CrA    P var.
V0541 CrA    P var?
V0545 CrA    VB. Combined brightness with a faint companion is given.
V0553 CrA    P var?
V0566 CrA    Min II 12.7.
V0568 CrA    Sometimes a cycle 60d - 80d.
V0569 CrA    Min II 13.1. EB type is possible.
V0571 CrA    Min II 14.7.
V0572 CrA    Min II 14.0.
V0577 CrA    Min II 13.2. RR type with twice shorter period is possible.
V0578 CrA    RV type with P = 118d is possible.
V0580 CrA    Min II 14.4.
V0595 CrA    P var.
V0601 CrA    Epoch of min is given.
V0603 CrA    Slightly noticeable Min II at the phase 0.5P.
V0604 CrA    d = 0.03P.
V0607 CrA    Min II 14.3.
V0612 CrA    d = 0.03P.
V0615 CrA    P var?
V0622 CrA    Sometimes 55d - 60d cycles.
V0633 CrA    P var.
V0634 CrA    Min II 13.9.
V0648 CrA    Min II is felt at the phase 0.5P.
V0659 CrA    P = 189.4d is possible.
V0667 CrA    In the region of the bright cometary nebula NGC 6729.
V0667 CrA    The spectral type is earlier than K.
V0676 CrA    RR type is possible.
V0686 CrA    Max I 5.34, Min I 5.41, Max II 5.35, Min II 5.40 [08970].
V0691 CrA    4U 1822-37. Emissions CIII/NIII lambda 4640 - 50,
V0691 CrA    He II lambda 4686, CIV lambda 1550 etc.
V0692 CrA    P = 0.83d is possible.
V0730 CrA    MinII 9.99 [011]. Type RRC with a twice shorter period is possible.
V0731 CrA    Large scatter on the light curve.
V0737 CrA    Multiperiodic, P2 = 0.156795d.
V0738 CrA    Globular cluster non-member?
V0739 CrA    Globular cluster non-member?
V0740 CrA    Globular cluster non-member?
V0741 CrA    P = 0.394d is also possible. Globular cluster non-member?
V0742 CrA    Globular cluster non-member?
V0743 CrA    Globular cluster non-member?
V0745 CrA    Globular cluster non-member?
eps   CrA    Min II 4.95.
R     CrB    IR excess.
S     CrB    OH, H2O, SiO maser.
T     CrB    VB? A (B <= 12m, 0.2"). SB (P = 227.6d).
T     CrB    The spectral period is present in the photometric data of
T     CrB    1891 - 1917 and 1960 - 1971 [08978]. The epoch of the first
T     CrB    outburst JD2402734 (1866). Two smaller outbursts were
T     CrB    observed in UV light, JD2438030 (1963) and 2442543
T     CrB    (1975) [08979].
U     CrB    Min II 7.72. P var.
RR    CrB    P2 = 377d. Delta(m) (P1) ~0.5m, Delta(m) (P2) ~0.6m.
RS    CrB    P2 = 69.5d [01100]. Main period oscillation: 9.1m - 11.6m.
RT    CrB    Nonlinear term: +2.01d*10**(-8)*E**2. Min II 10.52 (var).
RT    CrB    DII = 0.09P.
RV    CrB    P var. Max = 2428285.608 + 0.3316217d*E (JD2428285 - 31610);
RV    CrB    Max = 2431705.349 + 0.3317313d*E
RV    CrB    (JD2431705 - 32954); Max = 2433030.572 + 0.331705d*E
RV    CrB    (JD2433030 - 36814) [05496]; Max =
RV    CrB    2440001.453 + 0.331569d*E (1967 - 1971) [06237];
RV    CrB    Max = 2441451.413 + 0.331619d*E (1972 - 1974)
RV    CrB    [07032]. The Table gives current elements. On
RV    CrB    the period changes see also [03506]. Blazhko effect?
RW    CrB    d = 0.028P. Min II 10.29.
TW    CrB    Min II 11.0.
TZ    CrB    ADS 9979 A (B 6.72m, GIV, 6.6", 233deg, 1980).
TZ    CrB    SB2 (P = 1.139789d).
TZ    CrB    Epoch of Min is given. The variation presented in the
TZ    CrB    Table is superimposed by a second one, with the same
TZ    CrB    amplitude and P = 0.1d. The amplitude is given
TZ    CrB    for the combined light of ADS 9979 A and B, the
TZ    CrB    mean magnitude is for ADS 9979 A.
UU    CrB    During JD2444381.73 - .76 a slow flare was observed, with
UU    CrB    maximal amplitude 0.30m in the IK band and 0.18m in the
UU    CrB    U band.
AL    CrB    Spotted rotating G-type giant.
AR    CrB    MinII 11.44.
AS    CrB    MinII 11.75.
AV    CrB    MinII 12.41.
AW    CrB    According to [161], EW, P = 0.360920 d.
AY    CrB    Min II = 14.0.
BD    CrB    Min II = 14.6.
BG    CrB    VB AB (9.5m, 9.8m, 0.1", 192deg, 2007).
BR    CrB    Min II = 10.11.
CT    CrB    Strong Blazhko effect.
alf   CrB    lambda eff = 7230 A: DI = 0.034P, DII = 0.018P,
alf   CrB    Min II - Min I = 0.66P, depth of Min I 0.10m, Min II
alf   CrB    0.025m.
bet   CrB    VB A (B ~ 5m - 6m, 0.2",  ~130deg, 1978). SB (P = 3833.7d).
bet   CrB    Magnetic field var, P = 18.487d. The epoch of Min light
bet   CrB    is given.
gam   CrB    ADS 9757 (4.2m, 5.6m; A = 0.74", P = 91.0a).
U     Crv    VB A (B 13.5m, 0.4' p).
W     Crv    Min II 11.86. The light curve is asymmetrical, the maxima
W     Crv    differ in hight by 0.10m.
Y     Crv    Min II 11.7. RRC type with twice shorter period
Y     Crv    is possible.
Z     Crv    d = 0.06P.
RV    Crv    Elements do
RV    Crv    not satisfy some of the published moments of Min.
RZ    Crv    Min II 13.9.
SX    Crv    Min II 9.23. The shape of the light curve varies. Depth of
SX    Crv    Min I 0.20m, depth of Min II 0.18m. In 1972 the system
SX    Crv    became fainter than in 1971 by 0.06m.
TY    Crv    SB2.
XX    Crv    P1 is tabulated; P0 = 0.54452d.
XY    Crv    P1 is tabulated (amplitude 0.44m); P0 = 0.484820d (amplitude 0.28m).
R     Crt    Periods of light constancy which last up to 250d occur
R     Crt    every two or there thousand days. OH, H2O maser.
S     Crt    H2O maser.
T     Crt    Mean light var, P2 = 1006d.
V     Crt    Min II 10.1; Min II - Min I = 0.57P.
W     Crt    (k - b)2 = +0.21.
X     Crt    (k - b)2 = +0.02.
Z     Crt    d = 0.016P.
RR    Crt    P = 293d or 146d is possible.
RV    Crt    Min II 9.4:.
SU    Crt    [Fe/H] > -0.3.
SV    Crt    ADS 8115 A (B 11.5m vis, 1", 220deg). SB2 (P = 5.90513d,
SV    Crt    apsidal motion, P ~700a). Epoch of Min I in B light is
SV    Crt    given. Depth of Min II is 0.015m. EuII and SrII in
SV    Crt    emission.
AG    Crt    P varies.
AI    Crt    Blazhko effect, P=63d. The identification with NSV 5200 suggested in [153] is probably wrong.
AK    Crt    Min II = 11.15. The tabulated elements are for the eclipses. Pulsations: P = 0.067964d, with a variable amplitude up to 0.07m.
R     Cru    In the region of the open cluster NGC 4349.
T     Cru    In the region of the open cluster NGC 4349.
U     Cru    P var. Max = 2410143 + 351.4d*E (JD2410100 - 14100) [00237];
U     Cru    since JD2437600 - see Table.
W     Cru    Min II 9.3.
SU    Cru    [A/H] = -0.8.
SV    Cru    In the region  of the open cluster Ruprecht 97.
SV    Cru    Non-member of the cluster.
SW    Cru    VB A (B 14.0m, 12"). (k - b)2 = 0.27.
SY    Cru    d = 0.05P?
TU    Cru    Min II 11.5.
TW    Cru    Min II 12.85:.
TX    Cru    It is not excluded that actually P is much shorter,
TX    Cru    close to 1d, for instance.
TZ    Cru    P = 2.091140d?
UW    Cru    Min II 12.9; Min II - Min I = 0.536P.
UX    Cru    VB A (B 10"). Min II 12.4; Min I - Min II = 0.325P;
UX    Cru    DII = 0.025P.
VY    Cru    Min II 13.5.
VZ    Cru    P = 1.125810d?
WW    Cru    Min II 13.0.
WX    Cru    d = 0.040P. Light variability in maximum is noted.
WY    Cru    VB A. P = 9.013290d?
XX    Cru    P = 3.28566d?
XY    Cru    Min II 11.7.
XZ    Cru    P = 1.6495930d?
YY    Cru    Min II 13.0.
YZ    Cru    Min II 13.1.
ZZ    Cru    Min II 9.8.
AB    Cru    Min II 8.9.
AC    Cru    Min II 12.1.
AD    Cru    VB A (B 14.5m, 10", 270deg). P var. Max = 2434918.160 +
AD    Cru    6.39844d*E (JD2423800 - 35400) [02309];
AD    Cru    since JD2441000 - see Table.
AE    Cru    Depth of Min II 0.03m.
AF    Cru    Min II 9.87.
AG    Cru    The blue component is possible [09004].
AI    Cru    In the region
AI    Cru    of the open cluster NGC 4103. Min II 9.94.
AQ    Cru    Min II 13.8.
AT    Cru    Min II 12.6.
AW    Cru    Min II 13.9.
AY    Cru    Min II 11.2.
BB    Cru    Min II 14.0.
BC    Cru    Depth of Min II 0.03m.
BD    Cru    Depth of Min II 0.05m.
BF    Cru    Min II 12.3.
BH    Cru    Epoch of Min I is given in the Table. The light
BH    Cru    curve like the light curves of R Cen and R Nor
BH    Cru    has two maxima and two minima of different
BH    Cru    depths. Max I 7.6m (0.22P), Min II 8.0m (0.41P),
BH    Cru    Max II 7.2m (0.53P).
BI    Cru    Spectrum description [04949].
BK    Cru    In Coalsack region.
BM    Cru    In Coalsack region.
BP    Cru    3U 1223-62. A unique X-system. Consists of an X-pulsar
BP    Cru    with pulse period 698s [09018] moving on an excentric
BP    Cru    orbit (E = 0.47) around the ellipsoidal B2 supergiant with
BP    Cru    orbital period of 41.51d. Accretion of the stellar wind
BP    Cru    from the primary star on the pulsar increases during the
BP    Cru    periastron passage. Therefore large X-flares are observed
BP    Cru    with the elements: T (X Max) = 2433158.09 + 41.51d*E.
BP    Cru    Optical flares are possible.
BQ    Cru    B - V: +1.13, +0.88.
BS    Cru    In the open cluster NGC 4755.
BT    Cru    In the open cluster NGC 4755.
BU    Cru    In the open cluster NGC 4755.
BV    Cru    In the open cluster NGC 4755.
BW    Cru    In the open cluster NGC 4755.
DU    Cru    The identification with NSV 06012 (SIMBAD) is wrong.
EP    Cru    MinII - MinI = 0.62P.
EQ    Cru    MinII - MinI = 0.48P.
EW    Cru    A twice longer period is also possible.
FG    Cru    Multiperiodic.
FL    Cru    Multiperiodic.
bet   Cru    VB A (B 11.4m, 44.3", 322deg; C 7.5m, 372", 23deg).
bet   Cru    Interferometric binary. Multiple periods (the total V
bet   Cru    amplitudes of corresponding oscillations are indicated
bet   Cru    in brackets): P0 = 0.2365072d (0.034m), P1 = 0.160466d
bet   Cru    (0.029m), P2 = 0.121383d (0.01m), P02 = 0.249373d
bet   Cru    (0.016m), P13 = 0.24273d (0.024m), P24 = 0.23931d
bet   Cru    (0.028m), P03 = 0.16342d (0.016m), P14 = 0.16171d
bet   Cru    (0.029m).
tet 2 Cru    SB (P = 3.4380d). BCEPS, P > 1h? [08420].
lam   Cru    Type ELL with
lam   Cru    P = 0.7902d is possible. Amplitude and shape of
lam   Cru    the light curve vary. The secondary oscillation
lam   Cru    (A = 0.007m) with the elements Max = 2441779.034 +
lam   Cru    0.1793d*E is possible.
R     Cyg    VB A (B 9.3m, 91", 14deg). S4/6e - S8/6e.
T     Cyg    VB A (B 10.03m, 10.2", 122deg; C 12m, 13.6", 197deg).
U     Cyg    VB A (B 7.8m, 63.5", 51deg). P var. Max = 2406455 +
U     Cyg    461.57d*E (JD2404590 - 13900); Max = 2414827 +
U     Cyg    470.76d*E (JD2413900 - 19940); Max = 2421806 +
U     Cyg    455.95d*E (JD2419940 - 27380); Max = 2427848 +
U     Cyg    472.85d*E (JD2427380 - 35750); since JD2435750 - see Table.
W     Cyg    There is a second oscillation with P = 235.3d.
X     Cyg    P var. Max = 2410190.86 + 16.3841d*E (JD2410100 -
X     Cyg    23370) [09028]; since JD2417000 - see Table.
X     Cyg    There is a square term in the elements given in the Table:
X     Cyg    +1.01d*10**(-7)*E**2. [A/H] = 0.4.
Y     Cyg    Min II 7.75; E = 0.1458. Apsidal motion: P = 47.6 yr.
Y     Cyg    There are sinusoidal terms in the elements:
Y     Cyg    +0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E));
Y     Cyg    Min II = 2409454.9174 + 2.9963328d*E -
Y     Cyg    0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E)).
Z     Cyg    OH, H2O emission.
RR    Cyg    VB A (B 12.5m, 18.1", 58deg).
RS    Cyg    VB A (B 7.09m, 132", 355deg; C 9.3m, 56", 106deg).
RS    Cyg    Epoch of light minimum is given. The shape of the light
RS    Cyg    curve strongly varies. Double maxima are sometimes
RS    Cyg    observed (Min II at the phase 0.5P).
RU    Cyg    VB A (B 12.40m V, 10", 224deg; C 11.15m V, 19", 29deg).
RV    Cyg    VB A (B 10m, 142", 118deg).
RY    Cyg    In the region of the open cluster NGC 6883.
RZ    Cyg    The shape of the light curve strongly varies. Alternation
RZ    Cyg    of high and low maxima, as well as of shallow and
RZ    Cyg    deep minima is observed, as a rule: 9.8m <= Max <= 12.0m.
RZ    Cyg    11.8m <= Min <= 14.1m.
SS    Cyg    SB2 (P = 0.27512995d [08285]).
SS    Cyg    During maxima of brightness there are oscillations of
SS    Cyg    light and X-ray flux with amplitudes about 0.002m V
SS    Cyg    and periods changing between 7.29s and 10.90s [06102,
SS    Cyg    09032].
SU    Cyg    P var. Max = 2421278.503 + 3.845507d*E (JD2414250 -
SU    Cyg    29000) [01559]; Max = 2433095.944 + 3.845664d*E
SU    Cyg    (JD2429000 - 33150) [00921]; since JD2434500 - see Table.
SV    Cyg    VB A (B 9.5m V, 145", 140deg).
SW    Cyg    Min II 9.30; d(V) = 0.018P; d(U) = 0.00P. P var. Min I =
SW    Cyg    2414782.448 + 4.572937d*E (JD2411340 - 16450);
SW    Cyg    Min I  = 2418440.758 + 4.5727923d*E (JD2417060 -
SW    Cyg    19740) [00063]; Min I = 2421504.489 + 4.572729d*E
SW    Cyg    (JD2421470 - 24970); Min I = 2425185.550 + 4.5728386d*E
SW    Cyg    (JD2424960 - 29500); Min I = 2433160.669 + 4.5729841d*E
SW    Cyg    (JD2433000 - 36800) [09085]; Min I = 2438584.3081 +
SW    Cyg    4.57311736d*E (JD2438600 - 40560) [09085];
SW    Cyg    since JD2441160 - see Table.
SY    Cyg    d = 0.040P. Possible depth
SY    Cyg    of Min II 0.03m.
SY    Cyg    P var. Min I = 2411659.568 + 6.00584d*E (JD2411600 -
SY    Cyg    17100); Min I = 2420001.571 + 6.005716d*E
SY    Cyg    (JD2418760 - 20760) [01961];
SY    Cyg    Min I = 2437069.254 + 6.005626d*E
SY    Cyg    (JD2432800 - 37070) [05416].
SY    Cyg    Mean elements given in the Table represent epochs of
SY    Cyg    Min I in the interval JD2414400 - 37070 up to +- 0.07d.
SY    Cyg    According to [04248] the apsidal motion with the period ~46
SY    Cyg    years is possible.
SZ    Cyg    [A/H] = 0.5. P var [02392].
SZ    Cyg    Mean elements given in the
SZ    Cyg    Table represent epochs of Max up to  +- 0.5d. According
SZ    Cyg    to [09029] "the O - C diagram has a sinusoidal structure
SZ    Cyg    as is to be expected for a member of a binary system"
SZ    Cyg    with P orb = 65 years.
TT    Cyg    VB A (B 10.8m V, 70", 213deg; C 11.1m V, 83", 49deg;
TT    Cyg    D 10.7m V, 94", 268deg).
TV    Cyg    According to [03663] - spectrum G0.
TX    Cyg    [A/H] = -0.2. P var. Max = 2436793.138 + 14.708157d*E
TX    Cyg    (JD2415000 - 37000); since JD2436700 - see Table.
UU    Cyg    VB A (B 10.7m V, 3.6", 351deg).
UV    Cyg    VB A (B 10.8m V, 0.9", 79deg).
UW    Cyg    P var. Min I = 2419624.501 + 3.450797d*E (JD2410000 -
UW    Cyg    20750) [00526]; Min I = 2419624.501 + 3.450752d*E
UW    Cyg    (JD2419620 - 33000); Min I = 2433848.508 + 3.450740d*E
UW    Cyg    (JD2430000 - 41800); since JD2441800 -
UW    Cyg    see Table. Possible depth of Min II 0.05m.
UX    Cyg    P var. Max = 2432444 + 560.3d*E (JD2415670 - 32450);
UX    Cyg    Max = 2439352 + 578.0d*E (JD2432450 - 40500);
UX    Cyg    since JD2437600 - see Table. Sometimes rapid light
UX    Cyg    decreases on the ascending branch near Max are observed
UX    Cyg    [01563, 01564]. H2O, OH, SiO maser.
UY    Cyg    Delta(S) = 3.8.
UZ    Cyg    VB A (B 10.8m, 28", 130deg). d = 0.032P; Min II 10.31.
VV    Cyg    Min II 13.2. P var? [03665].
VW    Cyg    d = 0.035P; Min II 10.31. P var. Min I = 2417377.123 +
VW    Cyg    8.4305260d*E (JD2415660 - 17400); Min I =
VW    Cyg    2430444.061 + 8.4302826d*E (JD2417400 - 30450);
VW    Cyg    Min I = 2441116.868 + 8.4303917d*E + 4.31d*10**(-8)*E**2
VW    Cyg    (JD2430450 - 41120) [07096]; since JD2440350 - see Table.
VX    Cyg    [A/H] = 0.2. P var. There is a square term in the
VX    Cyg    elemenmts +8.02d*10**(-7)*E**2.
VZ    Cyg    P var. Max = 2437103.945 + 4.8645598d*E(JD2416000 -
VZ    Cyg    41000); since JD2434000 - see Table.
WW    Cyg    d = 0.008P; Min II 10.16. P var [06144]. Mean elements:
WW    Cyg    Min I = 2416981.299 + 3.3176924d*E (JD2412000 - 31000)
WW    Cyg    [00063]; since JD2431000 - see Table.
WZ    Cyg    Min II 10.9.
XX    Cyg    [Fe/H] = -0.49. P var. Max = 2430671.1010 +
XX    Cyg    0.134865026*E(2416560 - 30000); since JD2430000 - see
XX    Cyg    Table.
XZ    Cyg    [Fe/H] = -1.2. P var. Max = 2417201.241 + 0.4665878*E -
XZ    Cyg    0.000107d*10**(-6)*E**2 (JD2414000 - 35000) [02550];
XZ    Cyg    Max = 2438562.796 + 0.466570d*E (JD2434000 - 39800);
XZ    Cyg    Max = 2440445.789 + 0.466497d*E (JD2439800 - 41000)
XZ    Cyg    [06237]; Max = 2441453.3856 + 0.4664731d*E
XZ    Cyg    (JD2441000 - 42500) [07424]; Max = 2443028.641 +
XZ    Cyg    0.466438d*E (JD2442500 - 43800) [09101]; Max =
XZ    Cyg    2444142.650 + 0.466649d*E (JD2443800 - 44200)
XZ    Cyg    [09102]; since JD2444100 - see Table.
XZ    Cyg    Besides that the star has a strongly
XZ    Cyg    expressed Blazhko effect; the period of Blazhko effect
XZ    Cyg    varies, too [07424, 07425]. 0.13P <= M - m <= 0.22P;
XZ    Cyg    0.90m <= A(B) <= 1.70m, 0.70m <= A(B) <= 1.30m;
XZ    Cyg    -0.05P < O - C < +0.05;
XZ    Cyg    Max A = 2417025.5 + 57.401d*E (JD2417000 - 38500);
XZ    Cyg    Max A = 2438881.7 + 58.387d*E (since JD2438500).[09103].
XZ    Cyg    After JD2444000
XZ    Cyg    Blazhko effect period probably decreased to 56.3d [09102].
ZZ    Cyg    VB A (B 12.63m, 8.5", 43deg.
ZZ    Cyg    Total brightness variation range
ZZ    Cyg    is given. Min II 10.78. P var. Min I = 2417442.419 +
ZZ    Cyg    0.6286185d*E (JD2415000 - 25800) [07427];
ZZ    Cyg    since JD2427950 - see Table.
AA    Cyg    S 6/3.
AC    Cyg    H2O maser.
AD    Cyg    S 5/5.
AE    Cyg    d = 0.039P; Depth of Min II 0.06m.
AF    Cyg    Light curve (1914 - 1956) [09104].
AF    Cyg    Two more independent oscillations are superimposed:
AF    Cyg    P2 = 175.8d, P3 = 941.2d.
AK    Cyg    VB A (B 11.06m, A7, 20", 85deg).
AV    Cyg    P var. Max = 2420451.9 + 87.48d*E (JD2418782 -
AV    Cyg    24823); Max = 2427936.3 + 89.73d*E (JD2426326 -
AV    Cyg    28745); Max = 2429440.9 + 87.69d*E (JD2428820 -
AV    Cyg    31260); Max = 2436413.8 + 89.63d*E (JD2434610 -
AV    Cyg    37130); since JD2437450 - see Table.
AV    Cyg    0.27P <= M - m <= 0.50P.
AX    Cyg    VB A (B 10.2m, 18", 52deg).
AY    Cyg    In the region of the open cluster Dolidze 2.
BB    Cyg    P var. Max = 2426360 + 265.7d*E (JD2414900 - 26700);
BB    Cyg    Max = 2433091 + 258.6d*E (JD2426700 - 35500); Max =
BB    Cyg    2438354 + 266.9d*E (JD35500 - 40200) [09106];
BB    Cyg    since JD2439200 - see Table.
BF    Cyg    P orb = 750d [05655].
BF    Cyg    Irregular light variations and sometimes observed
BF    Cyg    brightenings by 2m - 3m are superimposed by semiregular
BF    Cyg    oscillations with the cycle 755d [01039, 08044].
BG    Cyg    P var. Max = 2421190 + 290.35d*E (JD2421150 - 29950);
BG    Cyg    Max = 2430546 + 307.3d*E (JD2429950 - 30850); Max =
BG    Cyg    2432872 + 289.5d*E (JD2430850 - 34920);
BG    Cyg    since JD2435100 - see Table.
BI    Cyg    VB A (B 9.4m, 126", 110deg).
BO    Cyg    D = 0.025P; Min II 12.0.
BR    Cyg    D = 0.020P; Min II 9.58.
BS    Cyg    SC 8/8. P var. Max = 2422655 + 420d*E (JD2422600 -
BS    Cyg    24750) [01161]; Max = 2425181 + 431.4d*E (JD2424750 -
BS    Cyg    26500) [01171]; since JD2437500 - see Table.
BY    Cyg    VB A (B 16m).
BZ    Cyg    [A/H] = 0.1. Double maximum.
CD    Cyg    [A/H] = 0.2. P var.
CD    Cyg    There is a square term in the elements:
CD    Cyg    +1.54d*10**(-6)*E**2.
CG    Cyg    VB A (B 11.8m, 1.3", 306deg; 1979.7).
CG    Cyg    10.10 <= Min II <= 10.44. P var.
CG    Cyg    Min I = 2422967.4248 + 0.63114347d*E
CG    Cyg    (JD2422900 - 38500); since JD2439000 - see Table. Combined
CG    Cyg    light range is given. Shape of the light curve varies
CG    Cyg    [08848].
CH    Cyg    Semiregular light variations with the mean cycle 97d;
CH    Cyg    mean brightness varies with the cycle ~4700d [01169].
CH    Cyg    There are also a cycle 725d [08849], rapid oscillations
CH    Cyg    (A <= 0.25m U) and flares [05350]. It is not excluded
CH    Cyg    that the system is an eclipsing one [06499].
CI    Cyg    d = 0.084P.
CI    Cyg    Depth of eclipses ~0.8m. The eclipses of B star are
CI    Cyg    observed. Usually there are light fluctuations near mean
CI    Cyg    brightness ( ~12.1m). The outbursts last some dozens
CI    Cyg    and hundreds days. Light curves [06155, 08044, 08850,
CI    Cyg    08851]. Emissions of H, He I, He II, [O III], and N III.
CM    Cyg    S 4/6.5e.
CU    Cyg    P var. Max = 2422643 + 223.8d*E (JD2422600 - 26500);
CU    Cyg    since JD2426500 - see Table.
CV    Cyg    dI = 0.06P; Min II 11.33. P var. Min I = 2424458.348 +
CV    Cyg    0.9834523d*E (JD2414300 - 24500); since JD2424450 - see
CV    Cyg    Table. Shape of the light curve and Min I depth vary.
CY    Cyg    SC 2/7.5.
CZ    Cyg    P var. Max = 2424500 + 284d*E (JD2424500 - 33600)
CZ    Cyg    [03122]; since JD2432700 - see Table.
DD    Cyg    P var. Max = 2425465 + 148.30d*E (JD2424800 - 39000)
DD    Cyg    [01149]; since JD2439000 - see Table.
DF    Cyg    P var [01177, 06107]. Mean
DF    Cyg    brightness varies: Min = 2411292 + 780.2d*E [01571].
DG    Cyg    SiO maser?
DH    Cyg    OH emission?
DK    Cyg    dI = dII = 0.04P; Min II 10.90. P var.
DK    Cyg    Shape of the light curve and depth of Min II vary.
DL    Cyg    Min II 9.9.
DM    Cyg    P var. Max = 2425887.560 + 0.4198557d*E (JD2415200 -
DM    Cyg    25900) [03506]; Max = 2425887.5597 + 0.41985715d*E
DM    Cyg    (JD2425880 - 29250) [00522]; Max = 2433872.420 +
DM    Cyg    0.41985842d*E (JD2429250 - 37900) [03506]; Max =
DM    Cyg    2438677.708 + 0.4198619d*E (JD2438600 - 41250)
DM    Cyg    [07114]; since JD2441240 - see Table.
DM    Cyg    There is also Blazhko effect with the elements:
DM    Cyg    Max(O - C) = 2442978.97 + 26.01d*E [08853];
DM    Cyg    -0.01 d< = O - C <= +0.01d. Delta(S) = 0.
DQ    Cyg    P = 180d?
DT    Cyg    P var. Max = 2424305.651 + 2.49913d*E (JD2424300 -
DT    Cyg    28500) [01183]; Max = 2432792.893 + 2.49934d*E
DT    Cyg    (JD2430000 - 36000); since JD2436000 - see Table.
DV    Cyg    P var. Max = 2425476 + 146.7d*E (JD2415200 - 29200);
DV    Cyg    since JD2432800 - see Table.
DW    Cyg    P var. Max = 2427603 + 279.6d*E (JD2416700 - 33500);
DW    Cyg    since JD2433500 - see Table.
DX    Cyg    Min II 14.2; Min II - Min I = 0.515P; DI = 0.22P,
DX    Cyg    DII = 0.12P.
DY    Cyg    VB A (B 3", 218 deg, 2002). Slow oscillations are superimposed by rapid ones with
DY    Cyg    A = 0.3m [03662]. According to [03148] type EB?
DY    Cyg    Min = 2436659.531 + 0.6990d(:)*E (JD2436600 - 37000)
DY    Cyg    [03148].
EE    Cyg    Min II 14.5.
EF    Cyg    142d <= P <= 175d.
EH    Cyg    P var. Max = 2427608 + 276.90d*E (JD2416200 - 27610);
EH    Cyg    since JD2427800 - see Table.
EI    Cyg    Epoch of Max I is given; heights of Max I and Max II
EI    Cyg    differ strongly, the depths of Min I and Min II are almost
EI    Cyg    equal. Max I - Min I = 52d.
EK    Cyg    Observations are represented by the elements in the
EK    Cyg    interval JD2425200 - 37900 only.
EM    Cyg    Mean cycle varies in the range 19d - 33d [04248, 09111].
EM    Cyg    Depth of eclipses 0.25m V; elements of eclipsing system
EM    Cyg    light variations: Min = 2437882.8595 + 0.29090950d*E -
EM    Cyg    21d*10**(-12)*E**2 [08854].
EM    Cyg    Sometimes there are light oscillations with periods
EM    Cyg    14.6s - 21.2s and an amplitude up to 0.4% [06102, 09112].
EN    Cyg    d = 0.012P. P var. Min = 2425181.311 + 2.2148998d*E
EN    Cyg    (JD2424880 - 29600) [00332]; since JD2433500 - see Table.
ES    Cyg    P var. Max = 2425146 + 157d*E (JD2425000 - 29300)
ES    Cyg    [00332]; since JD2432800 - see Table.
EV    Cyg    P var. Max = 2427740 + 259.1d*E (JD2425100 - 29100);
EV    Cyg    since JD2433500 - see Table.
EV    Cyg    The position of the star in the chart in [00530] is wrong
EV    Cyg    [00782].
EZ    Cyg    P var? Shape of the light curve and the amplitude
EZ    Cyg    strongly vary; 0.40P < = M - m < = 0.48P.
FF    Cyg    S 5.5/6-e.
FG    Cyg    P var. Max = 2426955 + 456.0d*E (JD2416000 - 27000)
FG    Cyg    [00001]; Max = 2426955 + 458.8d*E (JD2426900 - 34300)
FG    Cyg    [03122]; since JD2439200 - see Table.
FM    Cyg    P var. Max = 2425313 + 274d*E (JD2425300 - 29200)
FM    Cyg    [00332]; since JD2429200 - see Table.
FN    Cyg    P var. Max = 2429137 + 314.6d*E (JD2416200 - 29200)
FN    Cyg    [00001]; since JD2432800 - see Table.
FO    Cyg    A var. P var. Max = 2425193 + 156.6d*E (JD2425000 -
FO    Cyg    29200) [00332]; since JD2432500 - see Table.
FR    Cyg    Min II 14.0; d = 0.03P.
FT    Cyg    P var. Max = 2425184 + 156.7d*E (JD2425100 - 29200)
FT    Cyg    [00332]. 83d <= P <= 187d (JD2432500 - 38000).
FY    Cyg    P var. Max = 2425172 + 194.d*E (JD2425100 - 29300)
FY    Cyg    [00332]. 130d <= P< = 189d (JD2432500 - 38000).
GG    Cyg    d = 0.079P; Min II 12.1.
GM    Cyg    P var. Min = 2428754.305 + 4.745772d*E (JD2413200 -
GM    Cyg    33500) [01209]; since JD2433500 - see Table.
GN    Cyg    P var. Max = 2425448 + 156d*E (JD2425400 - 27400)
GN    Cyg    [01155]; since JD2427500 - see Table.
GO    Cyg    Min II 8.73. P var. Intrinsic light variability of the
GO    Cyg    components is possible [01210].
GS    Cyg    P = 195d?
GT    Cyg    Depth of Min II 0.05m? P var?
GY    Cyg    Secondary oscillation with P = 4000d and
GY    Cyg    A(V) = 0.5m is possible.
GZ    Cyg    Red.
HL    Cyg    d = 0.02P.
HV    Cyg    VB (Northern component).
HY    Cyg    P var. Max = 2425334 + 344d*E (JD2425300 - 29200)
HY    Cyg    [00332]; since JD2432760 - LB?
II    Cyg    P var. Max = 2425150 + 82d*E (JD2425120 - 25550),
II    Cyg    Max = 2425475 + 94d*E (JD2425550 - 29250) [00332];
II    Cyg    since JD2432500 77d <= P <= 99d.
IK    Cyg    P var. Max = 2425199 + 77.3d*E (JD2425000 - 29200)
IK    Cyg    [00332]; since JD2432500 - see Table.
IT    Cyg    P var. Max = 2425305 + 67.4d*E (JD2425300 - 850)
IT    Cyg    [00332]; since JD2432500 - see Table.
IU    Cyg    B - V: +0.90, +1.45. P var. Max = 2429157.6 + 31.22266d*E
IU    Cyg    (JD2417800 - 29250); Max = 2433601.3 + 31.1550d*E
IU    Cyg    (JD2432700 - 35400); since JD2435400 - see Table.
IV    Cyg    P var. Max = 2425470.406 + 0.33432871d*E (JD2425300 -
IV    Cyg    33120) [03506]; Max = 2434122.519 + 0.33433895d*E
IV    Cyg    (JD2432700 - 40200) [04248]; since JD2440200 - see Table.
IV    Cyg    Shape of the light
IV    Cyg    curve varies: 0.10P <= M - m <= 0.20P.
IX    Cyg    P var. Max = 2425173 + 172d*E (JD2425000 - 25900)
IX    Cyg    [00332]; since JD2428000 - see Table.
KL    Cyg    P var. Max = 2437906 + 536.8d*E (JD2418500 - 38000)
KL    Cyg    [00001]; since JD2438000 - see Table.
KP    Cyg    Delta(S) = 0.
KR    Cyg    Min II 9.37.
KU    Cyg    Min II 11.15; d = 0.047P. Shape of the light curve varies.
KV    Cyg    Min II 11.9.
KY    Cyg    H2O, OH maser.
LN    Cyg    Min II 14.3.
LO    Cyg    Min II 13.3.
LX    Cyg    P var. Max = 2432775 + 460.0d*E (JD2415000 - 33300)
LX    Cyg    [01159]; since JD2437900 - see Table. SC 7/9-e - SC 8/8.5e.
MQ    Cyg    VB A (B 17.5m B, 4.5", 122deg). P var. Max = 2432737 +
MQ    Cyg    428.5d*E (JD2414300 - 33300) [01229]; since
MQ    Cyg    JD2440000 - see Table.
MR    Cyg    Min II 9.12; d = 0.030P; DII = 0.19P.
MU    Cyg    Min II 14.4.
MY    Cyg    Min II 8.99. Min II - Min I = 0.5021P.
MZ    Cyg    P var. Max = 2427641.914 + 21.162460d*E +
MZ    Cyg    0.10575d*10**(-3)*E**2 (JD2414900 - 37900) [03689]; since
MZ    Cyg    JD2443600 - see Table. Probably it is an RV Tau type
MZ    Cyg    variable, and then the period should be doubled [08862].
MZ    Cyg    [A/H] = 0.1.
NQ    Cyg    EW type is possible. Close to V736 Cyg.
NU    Cyg    Min II 14.9.
NZ    Cyg    Min II 14.2.
OS    Cyg    P var.
OU    Cyg    Min II 15.6.
OY    Cyg    Star 23 - 30 [01321].
PP    Cyg    Star G in the chart for VV245 [07749].
PR    Cyg    Star 24 - 40 [01321].
PT    Cyg    Star 23 - 55 [01321].
PU    Cyg    Star 25 - 56 [01321].
PX    Cyg    Star 35 - 78 [01321].
PY    Cyg    Min II 15.2.
QS    Cyg    Min II 13.3.
QT    Cyg    Depth of Min II 0.04m.
QU    Cyg    Min II 15.1.
QW    Cyg    Min II 14.1.
QX    Cyg    Min II 14.5.
V0339 Cyg    np component of a close binary.
V0340 Cyg    Min II 14.5.
V0343 Cyg    [A/H] = -0.2.
V0346 Cyg    Companion 13.8m, 0.4' sf. Min II 11.9. P var.
V0346 Cyg    Min I = 2427270.241 + 2.743345d*E (JD2415000 - 32000);
V0346 Cyg    since JD2432000 - see Table.
V0348 Cyg    According to [07516] EW type variable with large
V0348 Cyg    irregularities: Min = 2441567.177 + 0.285768d*E
V0348 Cyg    (JD2441567 - 95).
V0355 Cyg    Min II 14.3.
V0360 Cyg    P var [06107]. Min I = 2429187.4 + 70.449d*E
V0360 Cyg    (JD2414600 - 34000) [00580]; since JD2426000 - see Table.
V0366 Cyg    Min II 10.2.
V0367 Cyg    VB A (A 0.1", 50deg; B 13.7m, 2.3", 255deg). Min II 7.16.
V0367 Cyg    Shape of the light curve and the radial velocity curve
V0367 Cyg    vary.
V0368 Cyg    According to [00204] EB type (12.8m - 13.8m pg)
V0368 Cyg    with the elements: Min I = 2425808.10 + 0.47586d*E
V0368 Cyg    (JD2425805 - 853).
V0369 Cyg    P var. Max = 2438199 + 104.46d*E (JD2426000 - 38200);
V0369 Cyg    since JD2438200 - see Table.
V0370 Cyg    Min II 11.9. P var. Min I = 2425096.429 + 0.77453979d*E
V0370 Cyg    (JD2414400 - 30000); since JD2430000 - see Table.
V0371 Cyg    Min II 12.5.
V0374 Cyg    d = 0.03P.
V0380 Cyg    Min II 5.76; Min II - Min I = 0.418P (1963).
V0380 Cyg    There are periodic terms in the elements:
V0380 Cyg    +0.8916d*sin(38.8deg + 0.0082deg*E) -
V0380 Cyg    0.0796d*sin(77.6deg + 0.0164deg*E) + 0.0088d*cos(26.4deg +
V0380 Cyg    0.0246deg*E); Min II = 2441262.266 + 12.425612d*E -
V0380 Cyg    0.8916d*sin(38.8deg + 0.0082deg*E) - 0.0796d*sin(77.6deg +
V0380 Cyg    0.164deg*E) - 0.0088d cos (26.4deg + 0.0246deg*E).
V0380 Cyg    Apsidal motion is possible with P = 1490 years.
V0382 Cyg    VB A (B 11.5m, 11", 332deg). Min II 9.12.
V0382 Cyg    Shape of the light curve and depth of Min II vary. P var.
V0382 Cyg    Min I = 2427992.458 + 1.885497d*E (JD2413480 - 29500)
V0382 Cyg    [01253]; since JD2428000 - see Table.
V0385 Cyg    Min II 12.4.
V0387 Cyg    Min II 11.6.
V0388 Cyg    Min II 9.15; d = 0.06P. P var. Min I = 2433584.540 +
V0388 Cyg    0.8590507d*E (JD2427600 - 37200);
V0388 Cyg    since JD2437200 - see Table.
V0389 Cyg    VB A (B 8.0m, 3.4", 305deg, 1980). SB (P = 3.313168d);
V0389 Cyg    Turns around the invisible third companion with
V0389 Cyg    P = 154.09d. According to [01256] the light varies with
V0389 Cyg    two alternate periods P1 and P2. The first oscillation
V0389 Cyg    (P1) with A = 0.19m satisfies the elements: Max =
V0389 Cyg    2423298.460 + 1.12912d*E, the second (P2) with A =
V0389 Cyg    0.05m - the elements: Max = 2429162.080 + 1.19328d*E.
V0389 Cyg    each of them continues for 1 - 3 weeks. At the transition
V0389 Cyg    from one oscillation to the other irregular light
V0389 Cyg    variations are sometimes observed or almost constant
V0389 Cyg    brightness. At the renewal of each oscillation its phase
V0389 Cyg    remains unchanged, experiencing no shift. According
V0389 Cyg    to [08909] in 1975 - 1977 periodicity was not observed.
V0393 Cyg    d = 0.02P.
V0401 Cyg    Min II 11.13. P var. Min I = 2432881.277 + 0.582717d*E
V0401 Cyg    (JD2428800 - 34000); since JD2434000 - see Table.
V0402 Cyg    VB A (B 20", 90deg).
V0407 Cyg    VB A (B 14.0m, 8", 190deg).
V0407 Cyg    Light variations of the Mira type
V0407 Cyg    variable are superimposed by the outburst of the probable
V0407 Cyg    nova which occured near JD2428400 (1936)
V0407 Cyg    with the consequent slow light decrease. Combined spectrum.
V0411 Cyg    P var. Max = 2421075 + 321d*E (JD2421000 - 31100)
V0411 Cyg    [01262]; since JD2431100 - see Table.
V0416 Cyg    Red.
V0425 Cyg    Description of the spectrum and its variations [02685, 03149].
V0427 Cyg    P var. Max = 2425471 + 143d*E (JD2425400 - 5950)
V0427 Cyg    [01155]; since JD2433850 - see Table.
V0429 Cyg    In the region of the open cluster NGC 6883.
V0430 Cyg    In the region of the open cluster NGC 6883.
V0430 Cyg    Max = 2425544 + 258d*E (JD2425500 - 27400) [01155].
V0432 Cyg    In the region of the open cluster Dolidze 3.
V0439 Cyg    In the region of the open cluster Berkeley 87 = OCL 161.
V0441 Cyg    Epoch of Min I is given.
V0442 Cyg    Min II 10.4:, d = 0.01P:. According to
V0442 Cyg    [08721] the period given in [00525] must be doubled.
V0443 Cyg    There is a periodic term in the elements:
V0443 Cyg    -0.016d*sin(0.00105*E).
V0444 Cyg    In the H II region S 109. Min II 8.06;
V0444 Cyg    D II  = 0.10P. P var. Min I  = 2430856.453 + 4.21238d*E
V0444 Cyg    (JD2415000 - 30000) [00007]; since JD2430000 - see Table.
V0445 Cyg    P var. Min = 2425527.391 + 1.947833d*E (JD2425500 -
V0445 Cyg    34700) [01155]; since JD2434700 - see Table.
V0447 Cyg    In the region of the open cluster NGC 6871.
V0448 Cyg    In the region of the open cluster NGC 6871. Min II 8.40.
V0450 Cyg    The light curve resembles that of DQ Her.
V0453 Cyg    In the region of the open cluster NGC 6871. Min II 8.68;
V0453 Cyg    d = 0.03P; Min II - Min I = 0.5077P. [07518]. According to
V0453 Cyg    [07518] there is apsidal motion with P = 71 years.
V0454 Cyg    Min II 12.3. In the region of the open cluster IC 4996.
V0455 Cyg    Min II 10.9. P var. Min I = 2431151.908 + 8.7689331d*E
V0455 Cyg    (JD2426800 - 33950) [01286]; since JD2436800 - see Table.
V0456 Cyg    Min II 11.4; Min II - Min I = 0.518P. P var?
V0457 Cyg    Min II 13.9.
V0458 Cyg    Min II 14.2.
V0461 Cyg    PB ~7000d? [08251].
V0462 Cyg    P var. Max = 2428540 + 376.0d*E (JD2416000 - 35200);
V0462 Cyg    since JD2435200 - see Table.
V0463 Cyg    Min II 10.65; Min II - Min I = 0.514P.
V0465 Cyg    There is a close companion of 17.5m.
V0466 Cyg    Min II 11.4.
V0469 Cyg    Min II 12.9; Min II - Min I = 0.57P.
V0470 Cyg    Min II 8.545.
V0471 Cyg    S 5.5/5.5.
V0473 Cyg    P var. Max = 2430615 + 218.5d*E (JD2418000 - 31000)
V0473 Cyg    [00346]; since JD2442300 - see Table.
V0474 Cyg    d = 0.014P.
V0477 Cyg    Min II 8.69; D II = 0.09P; d = 0.003P. P var. Min I =
V0477 Cyg    2429194.309 + 2.3470011d*E (JD2410000 - 29200)
V0477 Cyg    [00001]; Min I = 2437317.2695 + 2.3469943d*E
V0477 Cyg    (JD2429200 - 39700) [08919]; since JD2439700 - see Table.
V0477 Cyg    Apsidal motion with Pi = 349 years; E = 0.302 [06175].
V0477 Cyg    0.331P (1965 - 1970) <= Min II - Min I < = 0.460P (1904).
V0478 Cyg    VB A (B 12.8m, 4", 259deg. Min II 9.02; Min II - Min I =
V0478 Cyg    0.5072P.
V0482 Cyg    VB A (B 14.4m V, M4 III, 8", 225deg).
V0483 Cyg    Min II 11.9.
V0484 Cyg    Min II 13.6.
V0486 Cyg    Min II 14.3.
V0488 Cyg    Min II 13.0.
V0490 Cyg    Min II 13.5; Min II - Min I = 0.47P.
V0491 Cyg    Min II 14.7.
V0493 Cyg    Min II 12.9.
V0494 Cyg    Min II 13.6.
V0496 Cyg    Min II 12.5.
V0498 Cyg    Min II 10.27.
V0500 Cyg    VB B (A 11.5m; 18", 45deg). Min II 12.0.
V0501 Cyg    Min II 13.1; d = 0.02P.
V0502 Cyg    Min II 14.2.
V0505 Cyg    Min II 12.0.
V0509 Cyg    d = 0.05P.
V0512 Cyg    Min II 11.5. There is a periodic term in the elements:
V0512 Cyg    +0.065d*sin(0.2105263deg*(E + 538)).
V0513 Cyg    Min II 12.6.
V0519 Cyg    Min II 13.4.
V0520 Cyg    VB A (B 15", 135deg).
V0525 Cyg    d = 0.03P:.
V0526 Cyg    Min II 13.1. In the region of the open cluster TGC 7039.
V0532 Cyg    P var. Max = 2434618.158 + 3.283651d*E (JD2427900 -
V0532 Cyg    35000); Max = 2436817.694 + 3.282792d*E (JD2435000 -
V0532 Cyg    38700); since JD2438700 - see Table.
V0536 Cyg    d = 0.010P.
V0538 Cyg    B - V: +1.17, +1.50.
V0539 Cyg    P2 = 1500d.
V0541 Cyg    Min II 10.9; DII = 0.012P; Min II - Min I = 0.453P.
V0544 Cyg    P var?
V0546 Cyg    Min II 15.2:; Min II - Min I = 0.48P; d = 0.077P.
V0546 Cyg    In the dark nebula Barnard 144.
V0547 Cyg    B - V: +1.27, +1.73. In the dark nebula Barnard 144.
V0548 Cyg    Min II 8.62. P var. Min I = 2442279.3838 + 1.80524695d*E
V0548 Cyg    (JD2430800 - 42300) [08930]; since JD2442300 - see Table.
V0563 Cyg    P var. Max = 2427590 + 295.4d*E (JD2426000 - 30250);
V0563 Cyg    since JD2430250 - see Table.
V0567 Cyg    d = 0.036P.
V0581 Cyg    Red.
V0586 Cyg    In the region of the open cluster NGC 7039.
V0588 Cyg    VB A (B 18m, 15", 0deg). Very Red.
V0589 Cyg    VB.
V0606 Cyg    P var. Max = 2428376.7 + 50.245d*E (JD2427950 - 31330)
V0606 Cyg    [01262]; since JD2437100 - see Table.
V0612 Cyg    Cycles of 50 - 100d (JD2427950 - 31330) [01262];
V0612 Cyg    since JD2437100 - see Table.
V0614 Cyg    Min II 14.5.
V0618 Cyg    In the region of the open cluster TGC 7092.
V0622 Cyg    In the region of the open cluster NGC 7092.
V0628 Cyg    Min II 12.5.
V0635 Cyg    Min II 13.5.
V0643 Cyg    P var. Elements given in the
V0643 Cyg    Table are valid in the interval JD2427950 - 31330.
V0644 Cyg    VB A (B 15.6m, 6", 141deg; C 16.3m, 6", 141deg).
V0645 Cyg    Observed as the
V0645 Cyg    bright nebular condensation with ~2" diameter scattering
V0645 Cyg    light of an O8 star associated with it but invisible
V0645 Cyg    because of absorption. A part of strongly polarized
V0645 Cyg    bipolar nebula with diameter about 10". There are
V0645 Cyg    strong emission lines of H, Fe II, [O I], [S II], etc. In
V0645 Cyg    the spectrum [08942, 09129]. H2O maser source. Infrared
V0645 Cyg    source CRL 2789.
V0651 Cyg    Min II 14.7.
V0652 Cyg    Min II 12.1.
V0664 Cyg    d = 0.05P.
V0666 Cyg    P var. Max = 2427965 + 236d*E (JD2427950 - 31350)
V0666 Cyg    [01262]; since JD2433400 - see Table.
V0670 Cyg    sp component of a close binary.
V0680 Cyg    Min II 10.3.
V0685 Cyg    VB.
V0687 Cyg    Min II 10.4. P var?
V0688 Cyg    d = 0.029P.
V0690 Cyg    d = 0.021P.
V0691 Cyg    d <= 0.034P.
V0692 Cyg    Min II 14.9?
V0693 Cyg    Min II 14.4?
V0694 Cyg    d = 0.017P.
V0695 Cyg    31 Cyg. Probably enters a common system with V1488 Cyg
V0695 Cyg    (32 Cyg). VB A (B 13.0m, 36.8", 332deg; C 6.99m, 107.0",
V0695 Cyg    174deg; D 5.0m, 338", 323deg). d = 0.0151P.
V0695 Cyg    Interferometric binary eclipsing system (A = 0.08",
V0695 Cyg    E = 0.15 [01582]; 0.035", 141.8deg, 1980.4). The epoch of
V0695 Cyg    eclipse of the component of the spectral type B4 by the
V0695 Cyg    component of the type K4 is given in the Table. The
V0695 Cyg    amplitude strongly varies depending upon the wavelength:
V0695 Cyg    A(lambda 6560 A) = 0.03m, A(lambda 3530 A) = 1.80m [09131].
V0696 Cyg    Mean magnitude varies with P = 1600d.
V0700 Cyg    Min II 12.3. P var. Min I = 2432028.863 + 0.340047d*E
V0700 Cyg    (JD2431700 - 37500) [05352]; since JD2437500 - see Table.
V0704 Cyg    Min II 14.2.
V0706 Cyg    Min II 13.9.
V0713 Cyg    Min II 15.1.
V0720 Cyg    P var. Min I = 2427611 + 332d*E (JD2429450 - 32000)
V0720 Cyg    [00798]; since JD2432500 - see Table.
V0726 Cyg    Min II 12.8; d = 0.018P.
V0728 Cyg    P var. Min = 2425760.475 + 2.0601256d*E (JD2425500 - 35000)
V0728 Cyg    [00164]; since JD2439700 - see Table.
V0729 Cyg    VB A (B 13.5m, 1.5", 65deg). Min II 9.29. P var. Min I =
V0729 Cyg    2434264.638 + 6.597700d*E (JD2428700 - 37900)
V0729 Cyg    [00001]; since JD2439750 - see Table.
V0731 Cyg    VB.
V0735 Cyg    Depth of Min II 0.04m.
V0736 Cyg    Min II 16.5. Close to NQ Cyg.
V0737 Cyg    Star 23 - 50 [01321].
V0739 Cyg    Star 36 - 81 [01321].
V0741 Cyg    d = 0.03P.
V0742 Cyg    P var. Max = 2429409.448 + 0.93979d*E (JD2428420 -
V0742 Cyg    30700) [08977]; Max = 2431489.580 + 0.94010d*E
V0742 Cyg    (JD2430250 - 32350); Max = 2433282.014 + 0.93979d*E
V0742 Cyg    (JD2432350 - 33650); since JD2433650 - see Table.
V0742 Cyg    According to [08977] since JD2430700 the observations are
V0742 Cyg    better represented by the elements:
V0742 Cyg    Max = 2432943.701 + 0.93977897d*E - 1.067d*10**(-7)*E**2.
V0747 Cyg    The intervals between maxima of brightness
V0747 Cyg    are 2000 - 4000d. Not red.
V0751 Cyg    In the region of the nebula IC 5070. SB (P = 0.25d [09132]).
V0751 Cyg    Rapid small variations near maximum of brightness
V0751 Cyg    (B - V = +0.25) are superimposed sometimes by deep
V0751 Cyg    minima lasting for some hundreds days [02699]. Soft X-ray
V0751 Cyg    source [09133]. Spectrum description [02698, 09132].
V0752 Cyg    B - V = +0.77, U - B = -0.47.
V0753 Cyg    d = 0.12P. P = 0.952374d?
V0757 Cyg    Red.
V0758 Cyg    P = 400d?
V0759 Cyg    P var. Max = 2434513.427 + 0.36001476d*E
V0759 Cyg    (JD2414430 - 34570) [03506]; since JD2434500 - see Table.
V0759 Cyg    Blazhko effect.
V0779 Cyg    Type RR?
V0781 Cyg    P var?
V0783 Cyg    P var. Max = 2433261.029 + 0.62069487d*E
V0783 Cyg    (JD2424690 - 34000); since JD2438970 - see Table.
V0786 Cyg    Usually in minimum brightness, with rapid
V0786 Cyg    brightenings by 0.5m - 1.0m. In the interval JD2427692 -
V0786 Cyg    697 the brightness was 13.5m.
V0789 Cyg    P var? [Fe/H] = -0.91.
V0795 Cyg    sf component of a close pair.
V0796 Cyg    Min II 11.4.
V0797 Cyg    Min 15.4.
V0799 Cyg    P var.
V0801 Cyg    There is a square term in the elements:
V0801 Cyg    +1.93d*10**(-10)*E**2.
V0802 Cyg    P var. Max = 2432779.9342 + 0.59560377d*E
V0802 Cyg    (JD2425480 - 35170) [02775]; Max = 2439415.263 +
V0802 Cyg    0.5955638d*E (JD2435950 - 40000) [09266]. Max =
V0802 Cyg    2440036.409 + 0.595447d*E (JD2440000 - 41000); Max =
V0802 Cyg    2441517.498 + 0.595635d*E (JD2441000 - 42500);
V0802 Cyg    since JD2442500 - see Table. Shape of the light curve
V0802 Cyg    varies (0.13P <=  M - m <= 0.50P); period variations are
V0802 Cyg    accompanied sometimes by strong variations of amplitude
V0802 Cyg    (in the interval JD2440000 - 41000; 0.3m <= A <= 1.7m).
V0803 Cyg    Min II 14.5.
V0806 Cyg    Min II 15.0; DII = 0.061P.
V0807 Cyg    Min II 14.9.
V0808 Cyg    Brightness in maximum varies.
V0809 Cyg    Min II 13.6; DII = 0.069P.
V0810 Cyg    d = 0.050P. Depth of Min II 0.05m. P var?
V0817 Cyg    sp component of the pair.
V0818 Cyg    Shape of the light curve and period vary.
V0821 Cyg    Min II 15.6.
V0822 Cyg    Min II 13.0.
V0824 Cyg    Min II 14.3.
V0825 Cyg    Min II 16.9. Min II = 2433871.915 + 7.709015d*E.
V0826 Cyg    Min II 14.7.
V0828 Cyg    Min II 10.12.
V0832 Cyg    VB A (B 9.43m, 20", 352deg; C 11.62m, 27", 141deg; D 12.72m,
V0832 Cyg    38", 220deg). description of spectral variations [09135].
V0836 Cyg    Min II 8.77. P var. Min I = 2426547.5224 + 0.65341090d*E
V0836 Cyg    (JD2425500 - 42000) [03869]; since JD2441200 - see Table.
V0836 Cyg    Shape of the light curve varies.
V0840 Cyg    LS II 28.3deg [08090]. Cycles 250 - 300d.
V0841 Cyg    Min II 11.2.
V0842 Cyg    Min II 14.1.
V0844 Cyg    VB A (B 17.8m, 2.9", 50deg).
V0850 Cyg    Min II 11.8. P var. Min I = 2430587.263 + 4.5578d*E
V0850 Cyg    (JD2428750 - 30590) [04253]; since JD2434330 - see Table.
V0851 Cyg    d = 0.017P?
V0852 Cyg    Min II 14.9.
V0853 Cyg    Min II 14.2.
V0856 Cyg    Depth of Min II 0.05m.
V0857 Cyg    Depth of Min II 0.03m.
V0859 Cyg    Min II 12.1.
V0865 Cyg    Min II 14.6.
V0866 Cyg    Min II 13.9.
V0869 Cyg    Min II 14.8. Shape of the light curve varies.
V0870 Cyg    Min II 15.8.
V0871 Cyg    Min II 14.9.
V0873 Cyg    Min II 14.7. Min II - Min I = 0.48P.
V0874 Cyg    Min II 13.8.
V0877 Cyg    Min II 12.9.
V0880 Cyg    Min II 14.1; Min II - Min I = 0.506P; d = 0.02P.
V0881 Cyg    Delta(S) is small [09037].
V0882 Cyg    [Fe/H] = -1.42.
V0884 Cyg    np component of a pair. Min II 14.2.
V0885 Cyg    Min II 10.2.
V0886 Cyg    Min II 14.1; Min II - Min I = 0.515P.
V0887 Cyg    Depth of Min II 0.03m.
V0888 Cyg    Min II 15.9.
V0889 Cyg    Min II 10.4.
V0891 Cyg    Min II 9.4.
V0892 Cyg    Min II 15.5. nf component of a close pair.
V0900 Cyg    Min II 15.2.
V0902 Cyg    d = 0.02P. Depth of Min II 0.05m.
V0906 Cyg    Min II 15.7.
V0907 Cyg    Min II 14.9. According to [04427] Min I =
V0907 Cyg    2435066.257 + 0.54138554d*E.
V0908 Cyg    nf component of a close pair. Depth of Min II 0.04m.
V0909 Cyg    Min II 9.66.
V0910 Cyg    Min II 14.2; d = 0.02P.
V0911 Cyg    Min II 14.6. P var? Min I = 2432120.251 + 3.42262215d*E
V0911 Cyg    (JD2415500 - 37900) [04761]; since JD2437100 - see Table.
V0912 Cyg    Depth of Min II 0.05m.
V0913 Cyg    VB A (B 17m, 0deg).
V0920 Cyg    A var. Blazhko effect?
V0922 Cyg    d = 0.02P:.
V0924 Cyg    P var. Max = 2435706.776 + 5.5709816d*E (JD2432760 - 38000)
V0924 Cyg    [08053]; since JD2438000 - see Table.
V0925 Cyg    Min II 16.0.
V0927 Cyg    Epoch of Min brightness is given.
V0928 Cyg    Min II 15.4.
V0931 Cyg    Min II 14.5.
V0932 Cyg    Depth of Min II 0.04m.
V0934 Cyg    Min II 13.7.
V0936 Cyg    Depth of Min II 0.05m.
V0939 Cyg    Min II 12.5.
V0940 Cyg    Min II 15.1.
V0941 Cyg    Min II 13.2.
V0942 Cyg    VB A (B ~10deg, C ~110deg).
V0944 Cyg    np component of pair.
V0947 Cyg    Min II 15.0.
V0948 Cyg    Min II 15.2.
V0949 Cyg    Red.
V0955 Cyg    Min II 15.3. sp component of a close pair.
V0956 Cyg    Min II 15.1. sp component of a close pair.
V0957 Cyg    Min II 12.6.
V0958 Cyg    P = 199d?
V0959 Cyg    Min II 11.4; Min II - Min I = 0.52P; DII = 0.16P:.
V0959 Cyg    sp component of a close pair.
V0961 Cyg    Min II 12.4; Min II - Min I = 0.505P.
V0962 Cyg    d = 0.02P:.
V0964 Cyg    Min II 14.4.
V0965 Cyg    Min II 14.9. Type RRC? P = 0.32028628d?
V0970 Cyg    Min II 14.8.
V0974 Cyg    Min II 12.5; Min II - Min I = 0.462P.
V0974 Cyg    Min II = 2435373.398 + 3.204418d*E.
V0979 Cyg    Min II 14.7.
V0981 Cyg    Min II 15.0.
V0982 Cyg    Red.
V0997 Cyg    [Fe/H] = -0.77.
V1004 Cyg    Min II 13.0.
V1007 Cyg    Depth of Min II 0.04m.
V1008 Cyg    Min II 16.0.
V1010 Cyg    Depth of Min II 0.03m.
V1011 Cyg    Depth of Min II 0.04m.
V1012 Cyg    Min II 15.4.
V1016 Cyg    Before the outburst in 1964 the brightness
V1016 Cyg    changed between 15.0m and 17.5m pg [05701], the spectral
V1016 Cyg    type was late Me alpha [01222]. In the 1964 - 67 the
V1016 Cyg    brightness increased from 16.0m to 11.2m B. In 1967 - 69
V1016 Cyg    the brightness steadily increased to 10.05m B,
V1016 Cyg    being constant in V system (10.5m). In the infrared it
V1016 Cyg    changes in the limits 6.9 - 8.4 J, 4.7 - 5.8 K with the
V1016 Cyg    period 470d [07174, 09141]. High excitation emission
V1016 Cyg    spectrum with strong IR excess resembles that of
V1016 Cyg    symbiotic variables [09142]. X-ray and radio source.
V1018 Cyg    Min II 11.6.
V1021 Cyg    Min II 14.3.
V1023 Cyg    Min II 12.9; d = 0.03P:. DII = 0.14P.
V1023 Cyg    Min II - Min I = 0.495P.
V1024 Cyg    Depth of Min II 0.04m.
V1030 Cyg    Elements given in the
V1030 Cyg    Table are valid in the interval JD2426600 - 32300.
V1033 Cyg    P var.
V1034 Cyg    Min II 9.9.
V1035 Cyg    P var?
V1037 Cyg    Min II 14.8.
V1038 Cyg    VB B (9.4", 215deg, 1963). Min II 15.5.
V1039 Cyg    Min II 15.6.
V1042 Cyg    VB A (B 10m, 53", 110deg). In HII region S 109.
V1044 Cyg    Min II 16.5.
V1045 Cyg    Min II 16.0.
V1047 Cyg    d = 0.02P.
V1053 Cyg    d = 0.05P.
V1057 Cyg    In the dark nebula, in the region of the North America
V1057 Cyg    nebula (NGC 7000). In 1969 - 70 (JD2440400 - 830)
V1057 Cyg    the outburst from 16.5m to 10.3m occured. Brightness
V1057 Cyg    maximum was observed at JD2440830 (spectrum - B3).
V1057 Cyg    Before the outburst the light changed in the range
V1057 Cyg    15.5m - 16.5m, the spectral type was Ke with
V1057 Cyg    characteristic features of T Tau type stars [02698, 06415].
V1057 Cyg    After the outburst the brightness began to weaken
V1057 Cyg    monotonouosly and in 1982 reached 13.1m B (the spectral
V1057 Cyg    type about G2 - G5 Ib). Strong Halpha emission appeared
V1057 Cyg    in 1971. There are also small rapid light fluctuations.
V1057 Cyg    Description of light variations [06504, 07115,
V1057 Cyg    07754, 08996]. The star is associated with a luminous
V1057 Cyg    arc-shaped reflection nebula. This nebula with length
V1057 Cyg    of about 3' appeared in 1971 and its brightness is
V1057 Cyg    gradually decreasing simultaneously with the fading
V1057 Cyg    of the star.
V1061 Cyg    Min II 9.5.
V1063 Cyg    P var. Max = 2428260 + 339d*E (JD2428260 - 30700);
V1063 Cyg    since JD2433500 - see Table.
V1064 Cyg    Min II 15.3.
V1068 Cyg    Min II 11.2; d = 0.070P.
V1068 Cyg    A migrating wavelike distorsion with an amplitude ~0.1m V
V1068 Cyg    is being observed outside eclipses [08999].
V1073 Cyg    Min II 8.57.
V1074 Cyg    Min II 14.8.
V1083 Cyg    Min II 11.2.
V1085 Cyg    Observations given in [07010] contradict the elements given
V1085 Cyg    in [07193]: Min = 2437856.592 + 2.8089d*E.
V1096 Cyg    d = 0.03P.
V1102 Cyg    Radio-quiet N galaxy. Absorption spectrum without emission
V1102 Cyg    lines; z = 0.0272.
V1111 Cyg    Blazhko effect is possible.
V1122 Cyg    Blazhko effect is possible.
V1130 Cyg    Min II 12.9.
V1136 Cyg    Min II 13.2. Eccentric orbit (E = 0.3). Apsidal motion is
V1136 Cyg    possible [08051].
V1141 Cyg    Min II 11.8.
V1142 Cyg    Min II 13.4.
V1143 Cyg    Min II 6.06; Min II - Min I = 0.743P; d = 0.002P.
V1157 Cyg    Min II 13.6.
V1158 Cyg    d = 0.02P; Depth of Min II 0.04m.
V1161 Cyg    d = 0.01P.
V1162 Cyg    Only one Max was observed (see Table). Thereafter - either
V1162 Cyg    invisible, or fairly constant (17.6m - 17.8m). Bluish.
V1171 Cyg    VB A (B 11.0m, 0.34", 71.2deg; 1979.5). Min II 10.3.
V1175 Cyg    Min II 16.5. P var. Min I = 2434629.545 + 1.3330d*E
V1175 Cyg    (JD2426620 - 34630); since JD2434635 - see Table.
V1176 Cyg    VB. Variable is probably the northern red component.
V1187 Cyg    In the nebula IC 1318B. Min II 11.19. P = 3.7675d?
V1188 Cyg    Min II 14.3.
V1189 Cyg    Min II 13.7. P var. Min I = 2437906.516 + 1.041908d*E
V1189 Cyg    (JD2426620 - 31240); since JD2437906 - see Table.
V1191 Cyg    In the nebula IC 1318B. VB A (B 13m, 11", 299deg; C 13m,
V1191 Cyg    11", 284deg). Min II 11.11. Shape of the light curve varies.
V1193 Cyg    Min II 14.3.
V1196 Cyg    Depth of Min II 0.05m.
V1200 Cyg    Min II 16.1:.
V1210 Cyg    Red.
V1212 Cyg    Red.
V1218 Cyg    VB A (B 17m, sf).
V1225 Cyg    VB A (B 16m V, B - V = +1.3m, 1.2", 270deg; C 15.0m V,
V1225 Cyg    B - V = +0.5m, 2.4", 270deg); P var? Max = 2428250 +
V1225 Cyg    384.2d*E (JD2428200 - 38250) [03160]; since
V1225 Cyg    JD2438500 - see Table.
V1236 Cyg    Red.
V1255 Cyg    Brightness in Max varies in the range 15.2m - 16.0m with
V1255 Cyg    possible elements: Max = 2439382.281 + 0.28619537d*E.
V1256 Cyg    Min II 14.1.
V1273 Cyg    Min II 16.5.
V1275 Cyg    In the region of the open cluster NGC 6819.
V1281 Cyg    Min II 15.4.
V1285 Cyg    Red.
V1302 Cyg    Depth of Min II 0.05m.
V1305 Cyg    Min II 11.5m - 11.7m (var).
V1307 Cyg    Considerable dispersion of mean light curve points.
V1315 Cyg    Min II 15.3.
V1316 Cyg    (P) > 100d.
V1318 Cyg    LkH alpha 225. Associated with a cometary nebula.
V1321 Cyg    P = 0.7281802d?
V1322 Cyg    In the region of the open cluster NGC 6913.
V1326 Cyg    Min II 11.8; Min II - Min I = 0.53P.
V1327 Cyg    Very red.
V1329 Cyg    In 1891 - 1964 light variations in the range 14.2m - 15.5m
V1329 Cyg    with deep minima to 18m; the minima are satisfied by the
V1329 Cyg    elements given in the Table; D = 0.1p; spectral type M
V1329 Cyg    [07235]. In 1964 - the outburst up to 12.1m. Then gradual
V1329 Cyg    brightness decrease superimposed by periodical
V1329 Cyg    variations with an amplitude near 1m. Light minima
V1329 Cyg    as before are satisfied by the elements given in the
V1329 Cyg    Table but the character of eclipses changed (probably
V1329 Cyg    because of appearance of a dense envelope ejected
V1329 Cyg    by one of the components of the system). After the
V1329 Cyg    outburst high excitation emission spectrum with IR
V1329 Cyg    excess is observed similar to the spectrum of symbiotic
V1329 Cyg    variables.
V1331 Cyg    Associated with a cometary nebula.
V1334 Cyg    VB A (B 7.9m, B5 - B8, 0.13", 26.1deg, 1975).
V1336 Cyg    According to [07010], RR? P = 0.5d?
V1341 Cyg    Cyg X-2. SB1. Halo object (nu = -220 km/s). Strong
V1341 Cyg    reflection effect changes the spectral type of the F
V1341 Cyg    component. Spectral line profiles vary. The lines of
V1341 Cyg    He II, KCa II, C III,and N III are in emission. The
V1341 Cyg    system has low and high states. During the low state the
V1341 Cyg    mean light curve is a double wave with the range
V1341 Cyg    15.1m - 15.4m B. Epoch of Min I given in the Table
V1341 Cyg    corresponds to the F star in superior conjunction;
V1341 Cyg    Min II 15.4. The eclipse of the accretion disk at the
V1341 Cyg    phase 0.5P in partial. Rapid light variability by 0.1m
V1341 Cyg    in 10 minutes and by 0.5m in several hours is
V1341 Cyg    superimposed. In the high states lasting
V1341 Cyg    for ~10d the mean light increases by 0.5m. Radio
V1341 Cyg    source at 8085 MHz, source of soft and hard X-ray
V1341 Cyg    emission from 0.1 to 60 KeV.
V1345 Cyg    Min II 15.0:.
V1354 Cyg    Depth of Min II 0.04m.
V1356 Cyg    Min II 10.4.
V1357 Cyg    Cyg X-1. SB1. The epoch of the inferior conjunction of the
V1357 Cyg    optical component is given in the Table. Min II 8.88. The
V1357 Cyg    shape of the light curve varies; Min II sometimes are not
V1357 Cyg    observed. The periodicity in the light curve variations
V1357 Cyg    as well as in polarization changes is possible with
V1357 Cyg    P = 78.4d [09021, 09022]. Rapidly variable X-ray source in
V1357 Cyg    wide range up to 3 MeV characterized by the change of high
V1357 Cyg    and low states. Light and X-ray variation with P = 294d
V1357 Cyg    is also detected [09154, 09156]. Variable and flare radio
V1357 Cyg    source at 2695 and 8085 MHz.
V1372 Cyg    P2 = 360d?.
V1374 Cyg    Min II 17.7.
V1384 Cyg    In the region of the open cluster NGC 6913.
V1396 Cyg    VB AB (10.26m V, 12.3m V; A = 0.1127", P = 29.33 Y
V1396 Cyg    [09026]); mu = 0.67", P = 113deg; A-SB 2 (mAb - mAa = 0.6m,
V1396 Cyg    P = 3.275631d [09025]). Probably all the three components
V1396 Cyg    of the system are variables of the UV Cet type, and
V1396 Cyg    according to [05716] also of the BY Dra type. The range of
V1396 Cyg    combined brightness of the system is given in the Table.
V1396 Cyg    Really the flare of AB component was observed in the
V1396 Cyg    spectrograms [09025].
V1401 Cyg    Min II 13.6.
V1410 Cyg    P > 400d.
V1411 Cyg    P = 1.553478d?
V1412 Cyg    Min II 15.5.
V1414 Cyg    Northern component of a close pair; d = 0.04P.
V1416 Cyg    Min II 14.7.
V1417 Cyg    Min II 13.1.
V1421 Cyg    In the region of the planetary nebula NGC 6857 = K3 - 50.
V1425 Cyg    Depth of Min II 0.31m.
V1427 Cyg    In the region of the open cluster M39.
V1429 Cyg    Min II 15.3.
V1430 Cyg    Min II 15.0.
V1436 Cyg    Min II 15.9, D II = 0.08P; Min II - Min I = 0.48P.
V1437 Cyg    Min II 16.0.
V1440 Cyg    In the region of the open cluster NGC 6819.
V1465 Cyg    Resembles an eclipsing variable.
V1478 Cyg    VB A (B 17m:, 3", 80deg).
V1478 Cyg    Compact radio source. extended structure centered at the
V1478 Cyg    star is observed at 5 Ghz. Bq [] star with the excess of
V1478 Cyg    infrared radiation of dust at T = 300degK. Description of
V1478 Cyg    the spectrum [07080, 07081, 07523, 09159, 09160].
V1479 Cyg    In the region of the nebula IC 5070.
V1481 Cyg    Min II 12.5. In the region of the open cluster NGC 7128.
V1485 Cyg    Identical to VES 28, as it follows from latter star's
V1485 Cyg    coordinates and magnitudes in [7095], but the star is
V1485 Cyg    actually invisible in the chart in [7095], where a faint
V1485 Cyg    companion, to 0.4'N of the variable, is erroneously marked.
V1485 Cyg    Similarly, it is identical to +29deg 104, judging from the
V1485 Cyg    latter star's photometry and spectral type from [4732];
V1485 Cyg    however, the star is plotted slightly offset (by 0.8' to E)
V1485 Cyg    in the chart in [4732].
V1488 Cyg    32 Cyg. Probably enters a common system with V695 Cyg
V1488 Cyg    (31 Cyg). D = 0.015P, 0 < d < 0.011P. P var.
V1488 Cyg    Min I  = 2420670.0 + 1140.1d*E (JD2411400 - 29700).
V1488 Cyg    Since JD2429700 - see Table.
V1488 Cyg    The epoch of the eclipse of the B4 type
V1488 Cyg    Component by the K5 type component is given. There
V1488 Cyg    is also small physical light variability of the K
V1488 Cyg    component [08896, 09161]. Depth of eclipses depends of lambda:
V1488 Cyg    0.04M V, 0.13m B, 0.27m (lambda 4243A),0.90m (lambda 3552A).
V1489 Cyg    NML Cyg. 17.0m: - 18.0m V, B>21M; I - K = +8.17.
V1489 Cyg    Very large IR exess due to expanding gaseous-dust envelope.
V1489 Cyg    In the area 2.5"*3.5" around
V1489 Cyg    the star the system of about 60 discrete sources of
V1489 Cyg    OH emission is detected [07461]; source of OH, H2O,
V1489 Cyg    SiO maser emission. Light variations are periodical
V1489 Cyg    (see also [09163]). The object may be a protostar being
V1489 Cyg    observed at the end of condensation process. The late
V1489 Cyg    spectrum arises probably in the extending envelope
V1489 Cyg    [09165, 09166].
V1490 Cyg    In the region of the nebula IC 5070.
V1491 Cyg    In the region of the nebula IC 5070.
V1492 Cyg    In the region of the nebula IC 5070.
V1493 Cyg    In the region of the nebula IC 5070. V1707 Cyg 10.5"P.
V1494 Cyg    In the region of the nebula IC 5070.
V1495 Cyg    In the region of the nebula NGC 7000.
V1497 Cyg    In the region of the nebula NGC 7000.
V1498 Cyg    In the region of the nebula NGC 7000.
V1500 Cyg    In August 1975, before the very rapid increase
V1500 Cyg    of light, the brightness of the Nova gradually increased
V1500 Cyg    from 17.6m to 13.5m B (JD2442632 - 653.2). After Max
V1500 Cyg    almost monotonous decay of brightness is superimposed by
V1500 Cyg    light variations with the amplitude of 0.03m - 1.0m V;
V1500 Cyg    the period of these variations in the interval
V1500 Cyg    JD2442656 - 43100 changed in the range 0.1415d [09167,
V1500 Cyg    09168] - 0.137d [09169, 09170].  Since JD2443100 Min =
V1500 Cyg    2443696.4827 + 0.1396133d*E. Some investigators (see,
V1500 Cyg    for instance, [09173]) adopt double value of this peiod.
V1500 Cyg    A month after the light maximum of the Nova the
V1500 Cyg    radio emission was registered at 2695 and 8085 MHz [09171].
V1507 Cyg    The epoch of a broad Min I (superior conjunction of
V1507 Cyg    the B component) is given; Min II 7.01; D II = 0.20P,
V1507 Cyg    Min II - Min I  = 0.29P; e = 0.39. Unusual light curve
V1507 Cyg    [08213, 09049]. Shape of the light curve and depths of
V1507 Cyg    Min vary. Gaseous streams And expAnding envelope.
V1508 Cyg    Min II 13.3.
V1509 Cyg    VB A (B 11.7m, 55", 106deg).
V1511 Cyg    V - K = 13.6m.
V1513 Cyg    Gliese 781; mu alpha = -0.146S, mu delta = -1.00"; SB.
V1515 Cyg    In a dark nebula,  near the nebula NGC 6914. Connected
V1515 Cyg    with nebular appendage like a Comma. Light increase was
V1515 Cyg    observed from 1944 till 1958. Since 1958 the star is in
V1515 Cyg    Max. Slow light variations with A <= 1.6m. The absorption
V1515 Cyg    line Li I lambda 6707A is seen in the spectrum.
V1521 Cyg    Cyg X-3. Peculiar infrared X-ray source. V > 23m.
V1521 Cyg    Flare radio source. In the K band short and slow flares
V1521 Cyg    on the time scale about 2 minutes and 1-2 hours,
V1521 Cyg    irregular variations and longperiodic variability are
V1521 Cyg    observed [07752]. These variations are accompanied
V1521 Cyg    by periodical oscillations of infrared, X-ray and gamma
V1521 Cyg    radiation with the elements: Min = 2440949.8986 +
V1521 Cyg    0.1996830d*E + 1.25d*10**(-10)*E**2 [09187]. Usually the
V1521 Cyg    amplitude of these variations A(K) = 0.5m, but sometimes
V1521 Cyg    they disappear completely.
V1531 Cyg    LkH alpha 142. VB A (B = V1532 Cyg, 2.5", 90deg). In the
V1531 Cyg    region of the nebula IC 5070. Combined brightness and
V1531 Cyg    spectrum are given.
V1532 Cyg    LkH alpha 143. VB B (A = V1531 Cyg; B 2.5", 90deg).
V1532 Cyg    In the region of the nebula IC 5070. Combined brightness
V1532 Cyg    and spectrum are given.
V1535 Cyg    In the region of the nebula IC 5070.
V1536 Cyg    In the region of the nebula NGC 7000.
V1538 Cyg    In the region of the nebula NGC 7000.
V1539 Cyg    In the region of the nebula NGC 7000.
V1540 Cyg    In the region of the nebula NGC 7000.
V1546 Cyg    In the region of the nebula NGC 7000.
V1548 Cyg    VB A (B 16.7m, 6.2", 131deg).
V1554 Cyg    VB A (B 14.7m, 3.5", 214deg).
V1577 Cyg    In the cluster and nebula IC 5146.
V1578 Cyg    In the cluster and nebula IC 5146. VB A (B 15m, 5", 45deg;
V1578 Cyg    C 17m, 5", 225deg). Associated with a reflecting nebula.
V1580 Cyg    There is a periodic term in the elements:
V1580 Cyg    -0.027d*sin(0.045deg) (JD - 2439000).
V1581 Cyg    G 208 - 44. VB A (B = G 208 - 45, 15.97m V, M6Ve; 7.9",
V1581 Cyg    106deg, 1954; 8.2", 96deg, 1974). mu = 0.71", P = 140deg.
V1581 Cyg    The flare was observed during spectroscopic observations
V1581 Cyg    [09175]. The companion may be also a UV Cet type variable.
V1581 Cyg    The range of combined brightness variation of the system
V1581 Cyg    is given.
V1584 Cyg    Epoch of min brightness is given.
V1597 Cyg    In the region of the nebula IC 5070.
V1598 Cyg    In the region of the nebula IC 5070.
V1600 Cyg    In the region of the nebula IC 5070.
V1608 Cyg    In the region of the nebula NGC 7000.
V1610 Cyg    Infrared source CRL 2688, the star of the spectral type
V1610 Cyg    F5Ia, associated with a bipolar reflection nebula
V1610 Cyg    (the so-called Egg nebula). The northern component of
V1610 Cyg    the nebula is 4" to the north from the source. Since 1920
V1610 Cyg    to 1958 the integrated light of this component increased
V1610 Cyg    from 15.2m to 13.4b B and after that does not vary [08735]. Light
V1610 Cyg    of the faint (16.2m B) southern component (5" to the
V1610 Cyg    south from the source) varies by 0.6m B [09176]. The
V1610 Cyg    radiation of the nebula is strongly polarized (46%,
V1610 Cyg    theta = 106deg in V system). There are C3 absorption
V1610 Cyg    features as well as Na, C2, and [S II] emission in the
V1610 Cyg    spectrum. Probably the object is a precursor of a
V1610 Cyg    planetary nebula [09178].
V1611 Cyg    In the region of the nebula NGC 7000.
V1624 Cyg    A var.
V1624 Cyg    In 1957 out of a B star turned into Be star. Probably must
V1624 Cyg    be referred also to GCAS type.
V1661 Cyg    VB A (B 11.14m, 20", 174deg).
V1668 Cyg    There are sinusoidal light variations with A(V) = 0.15m
V1668 Cyg    and elements Min = 2443767.475 + 0.4392d*E in the
V1668 Cyg    descending branch of the light curve after JD2443765
V1668 Cyg    [09179]. Infrared light curves (1.6 - 10 mkm) have a
V1668 Cyg    secondary maximum (JD2443815) due to the formation of
V1668 Cyg    the dust envelope. At 10 mkm this secondary maximum is
V1668 Cyg    brighter than the primary one [09069].
V1669 Cyg    d = 0.036P.
V1671 Cyg    Delta(U) = 0.06.
V1674 Cyg    VB (B 15m, 5").
V1674 Cyg    The range of combined brightness variation is given. It
V1674 Cyg    is not excluded that it is the component B that is
V1674 Cyg    variable. Slow variations of mean brightness in the range
V1674 Cyg    10.555m - 10.570m B are superimposed by sinusoidal
V1674 Cyg    periodikal ones with P1 = 1.3608d (A1 = 0.0037m)
V1674 Cyg    and P2 = 0.8055d (A2 = 0.0032m).
V1676 Cyg    In the open cluster NGC 6871.
V1676 Cyg    ADS 13374 A (B 12.0m, 6.5", 64deg; C 11.0m, 9.5", 28deg
V1676 Cyg    D 9.5m, B3V, 11.4", 301deg; E 11.42m, 28.1", 109deg;
V1676 Cyg    F 7.36m, B1IA, 35.9", 29deg); SB2 (P = 112.7d).
V1696 Cyg    SB1 (Porb = 4.3174d). Epoch of Min brightness is given.
V1696 Cyg    The eclipse of the accretion disc around the compact
V1696 Cyg    object formed in the outburst of a Supernova in a binary
V1696 Cyg    system about 5*10**6 years ago is possible [03619].
V1701 Cyg    In the region of the nebula IC 5070.
V1702 Cyg    In the region of the nebula IC 5070.
V1703 Cyg    In the region of the nebula IC 5070.
V1704 Cyg    In the region of the nebula IC 5070.
V1706 Cyg    In the region of the nebula IC 5070.
V1707 Cyg    In the region of the nebula IC 5070. V1493 Cyg 10.5"f.
V1711 Cyg    In the region of the nebula NGC 7000.
V1716 Cyg    In the region of the nebula NGC 7000.
V1719 Cyg    Shape of the light curve varies.
V1720 Cyg    Min II 7.79.
V1721 Cyg    P var.Min I = 2442605.497 + 2.724370d*E (JD2442311 - 928);
V1721 Cyg    since JD2442928 - see Table.
V1722 Cyg    Min II 14.6?
V1726 Cyg    Possible member of an anonimous open cluster.
V1727 Cyg    4U 2129 +47. Lx/Lopt ~10.
V1727 Cyg    Emissions in the spectrum: NeII lambda 4686A, CIII - NIII
V1727 Cyg    lambda lambda 4640 - 50A.
V1735 Cyg    In the complex of dark nebulae associated with the
V1735 Cyg    open cluster and the nebula IC 5146. Lights up a
V1735 Cyg    reflecting nebula. Became brighter by 5m at least
V1735 Cyg    from 1952 to 1965.
V1737 Cyg    B - V = +3.7.
V1738 Cyg    B - V = +5.5:.
V1739 Cyg    B - V = +4.5:.
V1744 Cyg    Epoch of Max in U system is given.
V1746 Cyg    Sometimes P = 0.21d is observed.
V1747 Cyg    P > 100d. B - V = +4.0.
V1748 Cyg    In the nebula IC 1318a.
V1751 Cyg    In the nebula IC 1318c.
V1761 Cyg    Close companion? Elements are not certain.
V1860 Cyg    The chart in [68103] is wrong.
V2105 Cyg    Variability type and spectral type (F8Iab:) do not agree.
V2121 Cyg    Strong Blazhko effect.
V2150 Cyg    Type RR: is also possible.
V2174 Cyg    SB, Porb = 225.162d.
V2175 Cyg    X-ray source.
V2312 Cyg    Erroneously called HD 192776 in [190].
V2324 Cyg    Possible brightening trend over 6 years, maybe due to dissipating
V2324 Cyg    dust envelope, plus quicker variations.
V2363 Cyg    The depth of MinII is 0.13.
V2364 Cyg    MinII 11.73. O'Connell effect.
V2374 Cyg    The classification suggested in [276] is EB?, with a twice longer period.
V2375 Cyg    The depth of MinII is 0.20.
V2376 Cyg    The depth of MinII is 0.50.
V2380 Cyg    The depth of MinII is 0.35.
V2381 Cyg    The depth of MinII is 0.20.
V2383 Cyg    The depth of MinII is 0.15.
V2385 Cyg    The depth of MinII is 0.30.
V2386 Cyg    The depth of MinII is 0.50.
V2388 Cyg    The depth of MinII is 0.40.
V2389 Cyg    The depth of MinII is 0.35.
V2390 Cyg    The depth of MinII is 0.05.
V2394 Cyg    The depth of MinII is 0.16.
V2409 Cyg    MinII 14.1.
V2414 Cyg    MinII 10.22, the phase of MinII is about 0.3 P. Pulsations possibly overlapped.
V2417 Cyg    Cool companion, slow variations.
V2421 Cyg    MinII 14.20.
V2422 Cyg    The depth of MinII is 0.47.
V2428 Cyg    In quiescence, Max = 2440749 + 774 * E.
V2456 Cyg    MinII 11.6.
V2473 Cyg    VB AB (12.7mV, 14.3mr, 4", 267deg, 2000; C 14.4mV, 18", 188deg, 2000).
V2474 Cyg    A possible different classification is RV [100].
V2478 Cyg    VB A (B 17.1mpg, 12", 149deg, 1993).
V2486 Cyg    VB A (B 11.5m, 21", 248deg, 1998).
V2498 Cyg    Multiperiodic, P2 = 0.094d.
V2500 Cyg    Multiperiodic, P2 = 0.0677332d.
V2517 Cyg    VB A (B 14.1m, 5", 84deg, 1998).
V2533 Cyg    Multiperiodic, P2 = 0.162486d, P3 = 0.148877d.
V2534 Cyg    Multiperiodic, P2 = 0.171077d, P3 = 0.239556d. VB A (B 12.0, 3", 165deg, 2003; C 12.5, 10", 112deg, 2003; D 13.1, 16", 2931deg, 2003).
V2536 Cyg    VB B (A 9.7m; AB 7", 270deg, 2003).
V2541 Cyg    A twice longer period is also possible.
V2544 Cyg    Apsidal motion detected. The tabulated elements are for MinI. MinII = 2455005.5824 + 2.093799d x E.
V2547 Cyg    SB.
V2566 Cyg    Multiperiodic, P2 = 0.422d. Porb = 55.03d.
V2581 Cyg    Multiperiodic. P2 = 0.2486d, P3 = 0.09029d.
V2583 Cyg    VB A (B 19.4m, 0.6", 0deg, 2002).
V2608 Cyg    Multiperiodic. P2 = 0.091463d.
V2618 Cyg    MinII - MinI = 0.57P.
V2625 Cyg    VB A (B 5", 32deg, 1998).
V2642 Cyg    Total eclipses of the white dwarfs plus occasional small flares.
V2643 Cyg    O'Connell effect.
V2647 Cyg    MinII - MinI = 0.334P.
alf   Cyg    VB A (B 11.4m, 75.3", 106deg).
tau   Cyg    VB A (B 6.44m, G1V, A = 0.88", P = 49.80yr; C 12.20m,
tau   Cyg    29", 230deg). 0.083d <= P <= 0.125d.
tau   Cyg    The range of total light variation is given.
ups   Cyg    VB A (B 10.2m, 15.2", 220deg; C 10.2m, 21.5", 180deg).
khi   Cyg    VB A (B 10.8m, 158", 254deg). S 6 + %1e (Tc). SiO
khi   Cyg    maser. P var.Max = 2393559 + 405.88d*E (JD2337150 - 94000);
khi   Cyg    since JD2394000 - see Table.
P     Cyg    The appearance of the star was firstly noted in
P     Cyg    1600, when its brightness was 3m. Since the XVIII
P     Cyg    century the light of the star varies in the range
P     Cyg    4.6m - 5.6m vis. Radio source at the millimetre and
P     Cyg    centimetre wavelengths.
Q     Cyg    In minimum brightness varies periodically with the
Q     Cyg    amplitude 0.5m: Max = 2440495 + 54.99d*E; P = 64.81d is
Q     Cyg    also possible. Mean level of brightness varies in the
Q     Cyg    range 15.2m - 15.9m B.
S     Del    VB A (B 56", 342deg). Double maxima are sometimes observed.
U     Del    Mean brightness var, P = 1100d. According to [08993], the
U     Del    period value 160d - 180d is more likely than 110d.
W     Del    d = 0.017P. Min II 9.79. P var. Since JD2433000 - see
W     Del    Table. The light curve shape var.
RZ    Del    VB (A var; B var, 17", 137deg) [03771].
TT    Del    P var. Since JD2435000 - see Table.
TW    Del    Delta(m) var (0.5m + 3.4m).
TW    Del    The light curve resembles that of RV Tau, with Min I and
TW    Del    Min II; the epoch of Min I is given.
TW    Del    Min I = 2432171.1 + 118.4d*E (1947 - 1952);
TW    Del    Min I = 2435386.8 + 115.9d*E (1955 - 1963); during
TW    Del    1964 - 1970 - see Table.
TX    Del    P var. P = 6.166585d (JD2428000 - 36600); since
TX    Del    JD2436600 - see Table.
TY    Del    Min II 9.8. P var.Min = 2428020.399 + 1.191121d*E
TY    Del    (JD2428000 - 38000) [00279]; since JD2438000 - see Table.
TZ    Del    Epoch of Min is given.
VV    Del    Depth of Min II 0.05m.
YY    Del    Min II of the depth ~0.05m is possible. P var.
YY    Del    Min = 2425795.488 + 0.7930856d*E (JD2425000 - 34000)
YY    Del    [01329]; since JD2434000 - see Table.
AL    Del    Min II 12.4.
BG    Del    Min II 13.8.
BK    Del    P var?
BR    Del    Emission.
BX    Del    Delta(S) = 0.
BY    Del    Min II 11.8.
CE    Del    [Fe/H] = -0.68.
CF    Del    The light curve shape var?
CH    Del    [Fe/H] = -1.23. According to [09037], P = 0.315D.
CN    Del    Min II 14.6.
CR    Del    Min II 13.7.
CS    Del    [Fe/H] = -0.92.
CU    Del    Abrupt phase chande was noted.
CW    Del    P var.P = 0.58209d (JD ~2427100), P = 0.58211D
CW    Del    (JD ~2428800); During JD2429800 - 30600 - see Table.
DG    Del    The elements should be checked.
DK    Del    Min II 14.2.
DM    Del    Min II 8.80.
DT    Del    Epoch od Min is given. The elements are valid during
DT    Del    JD2425480 - 6260.
DX    Del    [Fe/H] = -0.11.
EG    Del    P var. Max = 2425535.42 + 0.3248545d*E (JD2425478 - 30619)
EG    Del    [00911]; abrupt change near JD2432578, since then see Table.
EI    Del    The mean brightness var, P ~600d.
EK    Del    B - V: +0.29, +0.53.
ES    Del    Epoch of Max from [03715], [07527] contradict the given
ES    Del    elements.
ET    Del    Min II 12.7.
EW    Del    Min II 15.5.
EX    Del    Min II 13.3.
FI    Del    Min II 14.5.
FK    Del    Min II 14.5.
FM    Del    Delta(S) = 0.
FP    Del    [Fe/H] = -1.44.
FR    Del    Min II 15.3.
FT    Del    Blazhko effect?
GG    Del    Min II 12.6. P var?
GN    Del    P var? Delta(m) var?
GY    Del    VB B (A = BD +15deg 4134A, SP A - F).
HR    Del    Porb = 0.170920d. The brightness began to increase on
HR    Del    JD ~2439653. Waves with maxima on JD2439752 (4.55m),
HR    Del    2439799 (4.64m), followed by a sharp main Max, flat max on
HR    Del    JD2439981 (4.09m) and final decline. Radio source.
HU    Del    mu = 0.685", theta = 79deg. Astrometric binary
HU    Del    (semiamplitude of deviations 0.118", Porb = 1.52yr).
II    Del    [Fe/H] = -1.30.
IO    Del    A single outburst  was observed (JD2439378 - 388).
IV    Del    D ~0.1d.
LS    Del    Min II 8.76.
OO    Del    MinII 18.03. A cluster foreground star.
OP    Del    MinII 17.33. A cluster foreground star.
OR    Del    VB AB (4" - 6"), SB2 Aa, Ab.
OX    Del    A twice longer period is not excluded.
del   Del    (k - b)2 = 0.19. SB2 (Porb = 40.58d; e = 0.7).
del   Del    Spectra of both SB components show Am features; Fe, Ca,
del   Del    Sc deficiency, Sr, Y, Zr, Ba, Ce, La, Eu excess.
del   Del    Both components are DSCT variables; the period of the
del   Del    main component pulsation is 0.158d, that of the
del   Del    secondary is 0.134d [07528]. Any of the oscillations may
del   Del    occasionally dominante in the combined brightness:
del   Del    according to [07529], Max = 2439338.4444 + 0.135547d*E;
del   Del    according to [07530], P = 0.154991d.
R     Dor    VB A (B 11.9m, 34", 10deg; C 11.0m, 35", 130deg, 1933).
R     Dor    H2O, SiO, HC3N emission.
S     Dor    VB A (B 12.1m, 13"). The member of the large magellanic
S     Dor    cloud. In the cluster NGC 1910 and a diffuse nebula.
S     Dor    One of the absolutely brightest stars. Deep Min: 1891,
S     Dor    1900, 1930, 1940, 1955, 1964.
T     Dor    VB A (B 12.0m vis, 5", 13deg.)
V     Dor    At the edge of the Large Magellanic Cloud.
RR    Dor    In the region of the Large Magellanic Cloud. Min II 14.5.
RW    Dor    In the region of the Large Magellanic Cloud.Cloud
RW    Dor    non-member. P var [09036]. Min II 11.2.
RX    Dor    In the region of the Large Magellanic Cloud. Cloud
RX    Dor    non-member?
SW    Dor    In the region of the Large Magellanic Cloud.
SW    Dor    Cloud non-member. P var [09036].
SX    Dor    In the region of the Large Magellanic Cloud,
SX    Dor    Cloud non-member. Delta(m) var.
SY    Dor    In the region of the Large Magellanic Cloud.
SY    Dor    According to [09036], variability is doubtful.
SZ    Dor    In the region of the Large Magellanic Cloud, cloud
SZ    Dor    non-member.
TY    Dor    In the region of the Large Magellanic Cloud, cloud
TY    Dor    non-member.
UU    Dor    In the region of the Large Magellanic Cloud,cloud
UU    Dor    non-member.
UV    Dor    In the region of the Large Magellanic Cloud,cloud
UV    Dor    non-member.
UX    Dor    In the region of the Large Magellanic Cloud, cloud
UX    Dor    non-member.
XX    Dor    In the region of the Large Magellanic Cloud, cloud
XX    Dor    non-member. [Fe/H] ~-1.3.
ZZ    Dor    In the region of the Large Magellanic Cloud, cloud
ZZ    Dor    non-member.
AA    Dor    d = 0.02P. Min II 11.21.
BE    Dor    In the field of the Large Magellanic Cloud.
BF    Dor    Min II = 13.2.
alf   Dor    VB A (B 4.3m, A = 0.2125", P = 13.00yr.)
alf   Dor    The range of combined brightness variations is given.
bet   Dor    P var. Current elements are given.
T     Dra    ADS 10937 A (B = UY Dra, optical, 16", 222deg).
U     Dra    P var. Mean elements are given.
W     Dra    P var. Max = 2416748 + 257.11d*E (JD2416750 - 21390);
W     Dra    Max = 2430826 + 262.11d*E (JD2421390 - 30820);
W     Dra    Max = 2439962 + 268.87d*E (JD2430820 - 40490);
W     Dra    since JD2440490 - see Table.
Y     Dra    According to visual observations, 7.8m - 15.0m.
Z     Dra    Min II 11.0. P var. Min = 2430973.314 + 1.3574176d*E
Z     Dra    (JD2428460 - 33300); Min = 2433268.708 + 1.357440d*E
Z     Dra    (JD2433300 - 43500); since JD2443500 - see Table.
RR    Dra    d = 0.015P. Min II 10.1. P var. Before JD2439000
RR    Dra    Min I = 2433390.458 + 2.83123d*E [01001];
RR    Dra    since JD2440000 - see Table.
RS    Dra    During JD2436012 - 37584 P = 145.3d.
RS    Dra    Delta(m) and the light curve share vary strongly.
RW    Dra    P var. Mean elements are given.
RW    Dra    Composite Blazhko effect;
RW    Dra    Pi = 93.95P = 41.61d; Pi1 = 280P; Pi2 = 6140P; Pi3 =
RW    Dra    3400P [01585]. 0.11P <= M - m <= 0.32P. Delta(S) = 3.
RX    Dra    Min II 10.3, d II = 0.009P.
RZ    Dra    Min II 10.38. P var. Min = 2429448.787 + 0.55087668d*E
RZ    Dra    (1907 - 1968) [03822]; since 1968 - see Table.
SU    Dra    P var. Before 1955 Max hel = 2420605.762 +
SU    Dra    0.66041890D; since 1955 - see Table. [Fe/H] = -1.39.
SW    Dra    Delta(S) = 3.5.
SX    Dra    d = 0.035P. Min II 10.0. P var. Min I = 2432273.276 +
SX    Dra    5.1692d*E (JD2432000 - 38000); since JD2442000 - see Table.
TT    Dra    P2 = 198d.
TW    Dra    ADS 9706 A (B 9.5m vis, 23deg, 3.6"). d = 0.02P;
TW    Dra    Min II 8.1. P var. Min I = 2433888.452 + 2.806870d*E
TW    Dra    (JD2433000 - 40000) [03825]; since JD2440000 - mean
TW    Dra    elements in the Table.
TX    Dra    Mean magnitude var, P2 = 654d.
UU    Dra    Mean magnitude var, P2 = 960d.
UX    Dra    According to [09086], the light curve may correspond
UX    Dra    to the type E; SB, P ~340d.
UZ    Dra    d = 0.01P; Min II 10.6. Possibly P = 1.65d [03827].
VW    Dra    According to photoelectric observations, 6.28m - 6.32m V.
WW    Dra    Nonlinear term: -4.98d*10**(-9)*E2.
WW    Dra    ADS 10152A (B 9.67m, 8.2", 5deg). Depth of Min II 0.08m.
WZ    Dra    Delta(m) var strongly.
XY    Dra    Min II 13.7.
XZ    Dra    P var. Before JD2438000 Max = 2427985.648 + 0.4764944d*E
XZ    Dra    [00188]. Epochs after JD2438000 are represented dy the
XZ    Dra    elements in the Table only on average. Blazhko effect;
XZ    Dra    according to [01474], Pi = 78d. [Fe/H] = -0.57.
ZZ    Dra    P var. Max = 2434509 + 274.5d*E (JD2416350 - 34600); since
ZZ    Dra    JD2437100 - see Table.
AE    Dra    Delta(S) = (4).
AF    Dra    VR var; SB?
AG    Dra    A soft X-ray source. Elements in the Table represent
AG    Dra    maxima in U band in 1974 - 1979 [09113].
AI    Dra    Min II 7.16, D II = 0.17P.
AP    Dra    Twice shorter period is possible.
AQ    Dra    Hbeta spectral line is probably filled in by emission.
AR    Dra    Min II 11.63.
AS    Dra    mu = 0.486", P = 289deg. SB. Delta(m) var.
AS    Dra    Large spatial velocity. The brightness
AS    Dra    varies with the phase of the orbital motion. Phases
AS    Dra    of Max and Min vary from cycle to cycle. The Table
AS    Dra    gives Porb [03075] and the epoch of the conjunction
AS    Dra    (G4 - star is behind).
AW    Dra    P var. since JD2430500 - see Table.
AX    Dra    Min II 11.0.
BE    Dra    Min II 11.5. The spectral type is late B.
BH    Dra    ADS 12019A (B Am, 9.25m, 10.8", 58deg). Min II 8.58.
BK    Dra    P var.Max = 2415150.817 + 0.592019d*E (JD2414900 - 16150)
BK    Dra    [00001]; since JD2416940 - see Table.
BK    Dra    Delta(S) = 8 in Max light.
BP    Dra    Min II 14.7.
BS    Dra    Min II 9.84.
BV    Dra    ADS 9537 A (B = BW Dra, 16.3", 358deg, 1980; C 12.69m).
BV    Dra    Min II 8.40.
BW    Dra    ADS 9537 B (A = BV Dra; C 12.69m). Min II 9.02.
BY    Dra    SB2 (Porb = 5.9750998d, e = 0.36). mu = 0.365", P = 150deg.
BY    Dra    Quasiperiodic variability :
BY    Dra    DM var, P var, (differential rotation), phase jumps.
BY    Dra    Flares up to Delta(U) = 1.07m.
CM    Dra    VB A (B SP = DC, 15.7m pg, 25.7", 22deg, common mu).
CM    Dra    mu = 1.619", p = 317deg, pi = 0.068", V nu = -118.6km/s.
CM    Dra    Min II 13.63. BY type variability: Delta(M) ~<= 0.05mV,
CM    Dra    P ~Porb. Flares: Delta(m) ~0.05.
CR    Dra    mu = 0.50", p = 168deg, pi = 0.048".
CX    Dra    SB, Porb = 6.69612d (with this period Delta(V) = 0.04m).
CX    Dra    Long-term cyclic variations: P ~2400d, Delta(V) ~0.2m.
CX    Dra    Flares ~0.1m. An X-ray source; the reflection effect is
CX    Dra    observed.
DE    Dra    d = 0.017P.
DG    Dra    Depths respective to Max I (Phase = 0.25); Min II 0.17m;
DG    Dra    Max II 0.01m.
DK    Dra    Porb = 64.44d.
DK    Dra    Epoch of Min is given. Both components show H and K CaII
DK    Dra    in emission.
DL    Dra    VB A (B 9.2m, 3.9", 318deg, 1982). P1 = 0.0825d, A1 =
DL    Dra    0.028m; P2 = 0.0837d, A2 = 0.026m.
DN    Dra    P = 109S. mu = 0.32", P = 153deg.
MU    Dra    MinII 12.08.
NO    Dra    A twice shorter period is not excluded. VB (8.4mHp, 9.6mHp, 0.1", 128deg, 1991).
NS    Dra    Min II = 11.43. MinII - MinI = 0.630: x P.
NT    Dra    Min II = 13.09.
NU    Dra    Min II = 11.06.
NV    Dra    Min II = 13.3 :.
NW    Dra    Min II = 13.45.
NX    Dra    Min II = 12.80. O'Connell effect.
OO    Dra    Min II = 11.55. Overlaid oscillations with an amplitude up to 0.04mB and a cycle about 0.027d.
OP    Dra    Min II = 15.00.
OQ    Dra    Min II = 14.1.
OR    Dra    Multiperiodic, P2 = 0.0826918d. VB AB (7.88, 8.81mHp; 0.1", 313deg, 1991).
OV    Dra    The star has a spectrum of a cataclysmic variable.
OX    Dra    Min II = 12.50.
OZ    Dra    The tabulated light elements are for eclipses. Flickering.
PQ    Dra    Min II = 14.05.
PR    Dra    Min II = 13.55.
PS    Dra    Min II = 13.3.
PT    Dra    Min II = 14.9 :.
PU    Dra    Min II = 12.25.
PV    Dra    Min II = 13.7.
PX    Dra    Min II = 6.88. VB A (B 10.8m, 18", 19deg, 2007).
PZ    Dra    Min II = 12.8.
QS    Dra    Biperiodic, P0 is tabulated. P1 = 0.0730446d.
QU    Dra    Min II = 14.6.
QY    Dra    Other possible periods: 0.603d; 1.205d (type EB).
V0338 Dra    Min II = 13.8.
V0339 Dra    Min II = 13.9.
V0341 Dra    Min II = 10.24.
V0342 Dra    Min II = 13.00.
V0343 Dra    Min II = 12.6.
V0344 Dra    Min II = 14.0.
V0354 Dra    A magnetic white dwarf with unusual properties. Variations are probably related to spots and axial rotation.
V0363 Dra    Fundamental period: see Table. First overtone: P1 = 0.40320d.
V0366 Dra    Multiperiodic, P = 0.0015926d is also excited.
V0368 Dra    Near the Draco dwarf galaxy; non-member.
V0372 Dra    O'Connell effect.
V0381 Dra    The tabulated light elements are for eclipses. Oscillations with P = 0.04407d and amplitudes 0.04mR, 0.05mV, 0.07mB, also present at both minima.
V0386 Dra    VB B (A 13.5mF; B 14.0mF, 8", 16deg, 2000); the tabulated range is for combined brightness.
V0388 Dra    O'Connell effect.
V0410 Dra    VB A (B 11.7mV, 8", 37deg, 2006).
V0413 Dra    VB AB (A 7.4m var, SB; B 10.2m, 0.5", 34deg, 2008).
V0414 Dra    Type ELL with a twice longer period is also possible.
V0416 Dra    Eclipses of about 0.2m in depth, Min = 2452368.53243 + 0.189109d x E.
V0425 Dra    MinII - MinI = 0.547:P.
V0432 Dra    MinII - MinI = 0.698P.
V0441 Dra    A twice shorter period is not excluded.
kap   Dra    IR excess.
phi   Dra    ADS 11311 (Delta(m) = 1.7m, 0.3", 288deg, 1967). A:SB, P =
phi   Dra    26.768d. The epoch of Max U light is given.
S     Equ    Min II 8.11. P var. Before JD2427000 Min =
S     Equ    2423746.490 + 3.4360050d*E [01140]; Min =
S     Equ    2437968.345 + 3.436072d*E (JD2427000 - 41000)
S     Equ    [03432]; since JD2441000 - see Table.
S     Equ    Gaseous streams; in Min light Halpha is in emission.
W     Equ    Min II 12.4. P var.
Z     Equ    A nearby star: 12.1m.
RT    Equ    P var strongly.
RW    Equ    Strong Blazhko effect.
RZ    Equ    Min II 12.2:.
SU    Equ    Min II 16.4.
SV    Equ    Depth of Min II 0.16m.
SW    Equ    Min II 15.6.
VV    Equ    Porb = 0.057083d.
gam   Equ    ADS 14702A (B 11.6m, 2", 268deg; C 12.6m, 48", optical).
gam   Equ    The Table gives the pEriod of oscillations. Data on the
gam   Equ    periodicity of the rotational variability of light,
gam   Equ    spectrum and magnetic field are contradictory
gam   Equ    (17.492d, 314d, 1785.7d, 72yr).
V     Eri    Mean magnitude var, P2 = 1209d.
W     Eri    SiO, OH, H2O maser.
Z     Eri    P2 = 746.4d.
RU    Eri    Min II 9.62.
RX    Eri    [Fe/H] = -1.32.
RY    Eri    d = 0.025P.
RZ    Eri    d = 0.018P. The depth of Min II 0.04m pg.
SV    Eri    [Fe/H] = -1.83. P var. P = 0.71365272d (JD2414000 - 21000);
SV    Eri    P = 0.71370172d (JD2421000 - 26000) [00862];
SV    Eri    Max = 2426590.319 + 0.7137406d*E (JD2426000 -
SV    Eri    34000) [09195]; since JD2434000 - see Table.
TT    Eri    (B - V)Max = +0.255m.
TV    Eri    (B - V)Max = +0.53m.
TZ    Eri    d = 0.015P. P var. Min = 2426066.198 + 2.606097d*E
TZ    Eri    (JD2426000 - 33500) [01490]; since JD2438200 - see Table.
UX    Eri    Min II 11.01. P var? Before JD2438500 Min I =
UX    Eri    2434368.570 + 0.4452820d [02494]; since JD2438500 - see
UX    Eri    Table.
UY    Eri    The shape of the light curve var. [A/H] = -1.6.
VW    Eri    Alternating P1 = 83.4d, P2 = 93.3d. Halo population.
WW    Eri    Min II 11.2.
YY    Eri    Min II 8.72. P var. Min I = 2433617.5198 + 0.321496212d*E
YY    Eri    (JD2433000 - 41500) [03850]; since 2441500 - see Table.
YY    Eri    X-ray source.
ZZ    Eri    Min II 14.4.
AN    Eri    Min II 14.9.
AO    Eri    d = 0.04P.
AS    Eri    Min II 8.42. X-ray source.
BB    Eri    (k - b)2 = 0.13.
BC    Eri    Min II 11.26:.
BK    Eri    Delta(S) = 8. P var.
BL    Eri    The elements should be checked.
BM    Eri    P > 20000d; D = 321d; d = 270d.
BM    Eri    Only one Min was observed. Outside Min, according to
BM    Eri    [05828], Delta(V) = 0.2m, Max = 2440643.0 + 30d*E.
BQ    Eri    Min II 10.9.
BV    Eri    Min II 8.42. dII = 0.06P.
BW    Eri    Min II 9.72.
BY    Eri    (k - b)2 = 0.06.
BZ    Eri    Min II 9.21.
CC    Eri    SB. mu = 0.310", P = 169deg, Pi = 0.083".
CC    Eri    Photometric P is close to Porb. X-ray source.
CI    Eri    VB (9.9m, 11.2m, 2", 106deg).
CO    Eri    Min II 9.1.
CS    Eri    (k - b)2 = 0.03.
CT    Eri    Min II 10.27.
CW    Eri    Min II 8.86, DII = 0.10P.
DL    Eri    P0 - see Table; P1 = 0.118795d [09206]; P2 = 0.0968d [09207].
DM    Eri    ADS 3380 (5.1m, 5.4m, 0.3", 161deg).
DM    Eri    Duplicity was observed only in 1877 and 1923.
DO    Eri    Epoch of Min is given. Oscillations with P ~6.14 Min, 7
DO    Eri    different frequencies have been found. Beat phenomenon,
DO    Eri    PB = 12.25d +-0.47d. Max of the oscillation amplitude
DO    Eri    almost coincides with Max of the magnetic field, the
DO    Eri    amplitude varies with Prot. Combined amplitude of
DO    Eri    oscillations 0.062m B.
DS    Eri    Min II 10.3. P var. Min = 2423147.25 + 0.827737d*E
DS    Eri    (JD2414869 - 23150); during JD2423150 - 31320 - see Table.
DW    Eri    ADS 3409 B (A 6.72m, G8III; B 9", 317deg).
DY    Eri    ADS 3093 C (A 4.43m V, K1V; B 9.51m V, DA, 82",
DY    Eri    105deg; BC A = 7", Porb = 252.1yr). mu = 4.05", P = 212deg.
DY    Eri    X-ray source.
DZ    Eri    Epoch is given for Max (y), Min (He I).
DZ    Eri    P = 3.67d is possible.
EF    Eri    2A0311 - 227. VB A (B 15.8m, 18", 260deg). mu alpha =
EF    Eri    +0.147", mu delta = -0.070".
EF    Eri    Epoch of narrow Min in IR light is given. The complex
EF    Eri    phenomenon of eclipses is described in [04041].
EF    Eri    Oscillations with P ~20.2 and 13.7 Min. [09211]. Flickering.
EG    Eri    Epoch of Min in Y light is given.
EH    Eri    ADS 3305 A (B 10.8m, 1.45", 60deg, 1917).
HV    Eri    Type RRC: is also possible.
KP    Eri    A twice shorter period is not excluded. VB (A 9.3m; B 9.6m, 0.8", 154deg, 1991).
KS    Eri    O'Connell effect.
KU    Eri    Multiperiodic. SB.
KV    Eri    Min II = 12.92. P varies. dP/dt = -0.20x10^(-5) d/yr.
KW    Eri    Min II = 13.85.
KX    Eri    Min II = 13.5.
KZ    Eri    Min II = 11.54.
LL    Eri    Amplitude(Min II)=  0.09mag.
LR    Eri    Blazhko effect, P = 122d [153].
LT    Eri    Eclipses with an amplitude about 1.6m.
LU    Eri    Min II = 17.7.
LW    Eri    Min II = 12.8.
MM    Eri    SB2, Porb = 13.5601d. VB AB (11.0m, 11.2m, 0.8", 79deg).
MQ    Eri    Min II = 12.7.
gam   Eri    ADS 2904 A (B 12.4m, 53", 242deg).
lam   Eri    Shell features are sometimes present in the spectrum.
mu.   Eri    SB, Porb = 7.35886d. Pulsational or rotational variations: P = 1.62592d, multiperiodic.
nu.   Eri    SB? P2 = 0.1735079d. Beat effect.
omi 1 Eri    P0 - see Table. P1 = 0.1291d.
tau 4 Eri    ADS 2472 A (B 9.9m, 6", 288deg; C 11m, 40", 99deg).
tau 9 Eri    SB1 (Porb = 5.954d). P = 1.2135d is not excluded.
S     For    VB (9.2m, 9.3m, 0.28", 358deg, 1964).
S     For    Found unusually bright only on one night
S     For    by three experienced observers in europe; harvard
S     For    photographs of the same night show it in normal brightness.
V     For    (B - V)Max = +0.26.
W     For    Min II is observed.
RX    For    (k - b)2 = 0.06.
RY    For    (B - V)Max = +0.535.
SS    For    (k - b)2 = 0.09.
SW    For    Delta(S) > 10:.
SY    For    SB2 [M + pec(eq)].
TZ    For    SB2. Possible P values:
TZ    For    37.805d; 44.18d; 50.46d; 75.61d. DI = 1d.
AV    For    VB AB (A 8.8m; B 10.0m, 1.5", 24deg, 1962; C 10.8m, 35", 102deg, 1931).
AZ    For    P0 is tabulated. P1 = 0.58823d.
R     Gem    VB A (B 11.4m pg, 173", 200deg, 1910). S 3.5/6e- S 6.5/6-.
S     Gem    VB A (B 11.1m, 70", 122deg).
T     Gem    S 3/4e.
U     Gem    Min = 2437638.82685 + 0.17690602d*E + 5.4d*10**(-12)*E**2
U     Gem    [09215]. Depth of Min 0.5m - 1.0m.
U     Gem    Spectrum description [09216].
V     Gem    P var. Max = 2407750 + 276.2d*E (JD2407700 - 15500);
V     Gem    Max = 2415729 + 278.3d*E (JD2415600 - 21600); Max =
V     Gem    2421839 + 269.8d*E (JD2421700 - 26500) [00458]; Max =
V     Gem    2432580 + 281.3d*E (JD2427500 - 32600); Max =
V     Gem    2434739 + 269.8d*E (JD2432600 - 35800);
V     Gem    since JD2435800 - see Table.
W     Gem    P var. Max = 2429815.990 + 7.914553d*E (JD2413200 -
W     Gem    31700); since JD2431700 - see Table. [A/H] = 0.2.
W     Gem    There is possibly faint blue companion.
RR    Gem    P var. Max = 2415219.734 + 0.39729235d*E
RR    Gem    (JD2412000 - 18000); Max = 2418278.900 + 0.39727274d*E
RR    Gem    (JD2418000 - 21000); Max = 2422865.229 +
RR    Gem    0.39724027d*E (JD2421000 - 25000) [09217]; Max =
RR    Gem    2427150.267 + 0.3972596d*E (JD2426200 - 27850);
RR    Gem    Max = 2434806.289 + 0.3973103d*E (JD2428200 - 34900)
RR    Gem    [02392]; since JD2436000 - see Table. Blazhko effect,
RR    Gem    PB = 48d [03618], PB = 37d [09221]. Delta(S) = 3.
RW    Gem    VB A (B 11.04m, 20", 105deg; C 11.84m, 100", 120deg).
RW    Gem    Min II 9.74; d = 0.02P.
RX    Gem    VB A (B 12.65m, 45", 215deg). Min II 9.28; d = 0.004P.
RX    Gem    P var. Min I = 2417970.0 + 12.20868d*E (JD2415000 - 27500) [07534];
RX    Gem    since JD2427600 - see Table.
RX    Gem    There is a square term in the elements given in the Table:
RX    Gem    +2.25d*10**(-7)*E**2. Luminous gaseous ring surrounds the
RX    Gem    primary component of the system [07535].
RY    Gem    VB A (B 12.30m, 45", 240deg). Min II 8.75; d = 0.023P.
RY    Gem    P var. Min I = 2418015.333 + 9.300876d*E
RY    Gem    (JD2418000 - 33000) [08653]; since JD2433000 - see Table.
RY    Gem    Component of A type is surrounded by a luminous gaseous
RY    Gem    ring.
RZ    Gem    VB. P var. Max = 2429632.453 + 5.529716d*E
RZ    Gem    (JD2415000 - 32400); since JD2432400 - see Table.
SS    Gem    9.9m <= Min II <= 10.7m.
SU    Gem    P var. Min I = 2429204 + 50.12d*E (JD2429200 - 355)
SU    Gem    [00310]; Min I = 2437772.5 + 50.39d*E (JD2437739 -
SU    Gem    39850); Min I = 2439856.6 + 50.10d*E (JD2439850 -
SU    Gem    40680); since JD2440680 - see Table.
SU    Gem    Mean brightness varies with the elements:
SU    Gem    Min = 2437953 + 680d*E; M - m = 264d.
SU    Gem    Amplitude of shortperiodical variations is 0.3m - 0.9m.
SW    Gem    Min brightness epoch is given.
SX    Gem    Min II 11.3; d = 0.05P:.
TX    Gem    Depth of Min II 0.04m; d = 0.017P:.
UV    Gem    VB A (B 19.5m, 7", 285deg).
WW    Gem    Min II 10.3.
WY    Gem    May be an eclipsing system similar to VV Cep. Atmospheric
WY    Gem    eclipse began probably in 1960 - 61, the mean phase of it
WY    Gem    being in 1968 [05730]. Variable magnetic field [01591, 04498].
WY    Gem    Intrinsic variability of blue component is also possible
WY    Gem    [07536].
YY    Gem    VB C (A 1.99m, B 2.85m, a = 6.06", P = 306.3 y; C 73",
YY    Gem    165deg, 1925); mu alpha = -0.0154s, mu delta = -0.108".
YY    Gem    Min II 9.59; Min II - Min I = 0.50P; D = 0.000P. X-ray
YY    Gem    source. P const [08655]. Both components are probably
YY    Gem    UV Cet type variables. Flare amplitude in the integrated
YY    Gem    light of the system reaches 0.3m V, or 1.8m U [09227].
AA    Gem    [A/H] = 0.0.
AC    Gem    Min II 11.3. P var. Min I = 2433649.30 + 1.661795d*E
AC    Gem    (JD2415000 - 36000) [01530]; since JD2430100 - see Table.
AF    Gem    VB A (B 14.8m, 2", 0deg). Min II 10.67.
AF    Gem    There is a square term in the elements given in the Table:
AF    Gem    -1.71d*10**(-10)*E**2.
AH    Gem    Min II 14.8:.
AI    Gem    Min II 14.0.
AL    Gem    Min II 9.85.
AN    Gem    Min II 13.3:; d = 0.037P.
AU    Gem    OH emission.
AV    Gem    Min II 12.8:.
AY    Gem    Min II 10.9.
AZ    Gem    Min II 12.4.
BB    Gem    VB A (B 12m, 25", 270deg).
BP    Gem    P var. Max = 2434120 + 243.9d*E (JD2418700 - 36600);
BP    Gem    since JD2436600 - see Table.
BT    Gem    Min II 14.0:.
CI    Gem    UG?
CM    Gem    Min II 15.0.
DL    Gem    VB A (B 13.1m, 18", 180deg).
DN    Gem    VB A (B 13.5m, 12", 16deg; C 12.0m, 80", 99deg).
DP    Gem    Min II 14.0. RRC? P = 0.2792d?
DX    Gem    P var. Max = 2433182.876 + 3.136226d*E (JD2425000 -
DX    Gem    34000); Max = 2435554.199 + 3.136955d*E
DX    Gem    (JD2434000 - 36500) [08300]; since JD2436500 - see Table.
EF    Gem    P var. Min = 2428108.49 + 6.10222d*E (JD2428500 -
EF    Gem    42800) [00407]; since JD2442800 - see Table.
EL    Gem    Min II 13.6.
EN    Gem    Min II 13.8.
EW    Gem    P var. Max = 2428495.686 + 0.523750d*E (JD2428100 - 30780);
EW    Gem    since JD2430780 - see Table.
EY    Gem    Min II 13.0.
FT    Gem    Min II 14.1.
GP    Gem    Min II 13.5.
GR    Gem    15.6 <= Min II <= 15.9.
GW    Gem    Min II 10.68.
GX    Gem    Min II 11.3.
GZ    Gem    P = 1.225290d?
HH    Gem    Min II 13.8.
HR    Gem    Min II 11.7.
HY    Gem    Min II 17.5.
II    Gem    P = 223d?
IP    Gem    Min II 14.5.
IR    Gem    In supermaxima there are superhumps with P = 102 Min
IR    Gem    [09232].
IZ    Gem    D >= 0.24d.
KN    Gem    The minor planet (123) Brunhild.
KQ    Gem    Min II 14.6.
KU    Gem    d = 0.05P.
KV    Gem    Epoch of Min of brightness is given. EW
KV    Gem    type is possible according to the spectrum [09037].
KZ    Gem    The cycle may be 129d.
LM    Gem    d = 0.02P.
LX    Gem    Red.
MO    Gem    Red.
MP    Gem    VB.
MU    Gem    Min II 14.9.
MZ    Gem    Min II 16.7.
NQ    Gem    In the spectrum of the carbon
NQ    Gem    star the hydrogen emission lines and ultraviolet
NQ    Gem    continuous emission appeared in February 1970 [06348].
NY    Gem    HD 47396 (Pec) = S 5438 = CSV 798 = CSV 6468.
NY    Gem    In the chart in [00156] the position of the variable is
NY    Gem    wrong.
OS    Gem    Oscillations with
OS    Gem    the period P1 given in the Table are superimposed
OS    Gem    by oscillations with the period P0 = 0.070d and smaller
OS    Gem    amplitude. P1/P0 = 0.78.
V0345 Gem    The variability may be due to the fainter (B) component.
V0371 Gem    Erroneous identification with HD 256211 in the literature is due to large positional errors in the HD catalogue for this field.
V0372 Gem    The depth of MinII is 0.22.
V0373 Gem    MinII 9.39.
V0375 Gem    MinII 13.4.
V0383 Gem    VB A (B 15.2mV, 12", 212deg, 1998; more companions at larger distances). The tabulated amplitude was influenced by the companions.
V0396 Gem    Min II = 10.37:.
V0399 Gem    Min II = 10.44.
V0400 Gem    Min II = 11.90.
V0401 Gem    Min II = 12.55.
V0402 Gem    Min II = 12.35.
V0403 Gem    Biperiodic, second period 0.1534d.
V0404 Gem    Min II = 12.9.
V0405 Gem    Min II = 10.97.
V0409 Gem    Min II = 13.9.
V0410 Gem    Min II = 11.06.
V0411 Gem    The depth of MinII is 0.26 mag (*).
V0412 Gem    The depth of MinII is 0.5 mag (*).
V0413 Gem    The depth of MinII is 0.40 mag (*).
V0414 Gem    Min II = 10.71.
V0415 Gem    Min II = 12.8.
V0416 Gem    Min II = 13.1.
V0418 Gem    Intermediate polar. Porb is tabulated, Pspin = 480.7080s.
V0421 Gem    Min II = 15.3.
V0422 Gem    Min II = 8.28.
V0425 Gem    Min II = 12.78.
V0428 Gem    Min II = 11.07.
V0432 Gem    Type EW with a twice longer period is also possible.
V0435 Gem    The depth of MinII is 0.35 mag (*). O'Connell effect.
zet   Gem    VB A (B 11.46m, 87", 84deg; C 7.56m, 97", 350deg). P var.
zet   Gem    Max = 2410640.42 + 10.15477d*E (JD2394600 - 2407150);
zet   Gem    Max = 2422366.187 + 10.15288d*E (JD2407150 - 22300);
zet   Gem    Max = 2426802.918 + 10.15172d*E (JD2422300 - 34500)
zet   Gem    [02392]; since JD2434500 - see Table.
zet   Gem    All the observations are satisfied also by the
zet   Gem    elements: Max = 2443785.444 + 10.150135d*E -
zet   Gem    5.24d*10**(-7)*E**2 [09029].
zet   Gem    May by a DCEPS type variable.
eta   Gem    VB A (B 8.8m, GO III - IV, 1.60", 269.4deg, 1977). SB1
eta   Gem    (P = 2983d [09236]). Epoch of Min brightness is given.
eta   Gem    The deepest minima (corresponding to the middles of the
eta   Gem    descending branches of the radial velocity curve) are
eta   Gem    satisfied by the elements: Min = 2429355 + 2984d*E
eta   Gem    [01551].
mu.   Gem    VB A (B 9.8m, 122", 141deg).
sig   Gem    VB A (B 10.8m, 182", 316deg); SB1 (P = 19.603d [09238]).
sig   Gem    There is a Min II on the light curve; Min II sometimes
sig   Gem    disappears and sometimes becomes deeper then Min I.
sig   Gem    Min II - Min I = 0.5P.
U     Gru    Depth of Min II 0.05m. d = 0.011P.
W     Gru    P var. Nonlinear term: +7.84d*10**(-9)*E**2. Min II 10.0.
X     Gru    d = 0.008P. Min II 10.69. P var.
X     Gru    Current elements are given.
Z     Gru    Delta(S) = 12:.
Z     Gru    The shape of the light curve and P are strongly variable.
RS    Gru    (k - b)2 = 0.22.
RT    Gru    (k - b)2 = 0.02. Blazhko effect.
RV    Gru    (B - V)Max = +0.93. Min II 11.4.
RW    Gru    Delta(S) = 10. Blazhko effect.
RX    Gru    Min II 10.7.
RY    Gru    Superposition of irregular variations?
RY    Gru    During JD2434513 - 517 precalculated minima were not
RY    Gru    observed.
RZ    Gru    A description of light changes [02809].
UW    Gru    [Fe/H] = -1.6.
VW    Gru    P >= 260d?
VY    Gru    P > 160d.
VZ    Gru    RR type is also possible.
AK    Gru    Elements should be checked.
AP    Gru    P var. Mean elements JD2427992 - 36848 - see Table.
AP    Gru    during JD2434250 - 36848 Max = 2434337.337 + 0.5082945d*E.
AR    Gru    Min II 10.6.
AV    Gru    P >= 160d is possible.
AW    Gru    Min II? JD2436818.
BC    Gru    Min II 10.3. RRC type is possible.
BD    Gru    Min II 14.9.
BH    Gru    Min II 15.2:.
DV    Gru    A twice longer period is not excluded.
DW    Gru    VB (A 11.8mV; B = GSC 8449.00117, 13.0mB, 13", 334deg, 1999; component A varies? [063]). Combined magnitudes are tabulated. MinII - MinI = 0.44P.
EN    Gru    P varies. dP/dt = +0.55 x 10^(-5) d/yr.
pi. 1 Gru    VB A (B 10.9m, G0V, 2.7", 202deg).
T     Her    VB A (B 10m, 67", 321deg).
U     Her    SiO, OH, H2O maser.
W     Her    ADS 10121 A (B 14.2m, 6", 334deg).
X     Her    P2 = 746d.
Z     Her    VB A (B ro > 10"). Min II 8.18.
Z     Her    nonlinear term: -6.19d*10**(-10)*E**2.
RU    Her    SiO maser. The spectrum in Min
RU    Her    light is composite; a companion? [03502].
RX    Her    Min II 7.74.
SW    Her    B - V; +0.12, +0.40. P var. Before 1921 Max =
SW    Her    2416687.018 + 0.4928864d*E.
SX    Her    [Fe/H] = -1.8.
SY    Her    On period variations see [08699].
SZ    Her    Min II 10.10. P var. Min = 2430766.8390 + 0.818096d*E +
SZ    Her    0.0165d*sin(0.010465deg*E + 180deg) [05749].
SZ    Her    The Table gives current elements satisfac -
SZ    Her    tory after JD2438000.
TT    Her    Min II 9.89. The light curve shape var.
TT    Her    P var. Before JD2430000 Min = 2425433.627 +
TT    Her    0.9120846D [02389]; Min = 2434525.2572 + 0.9120800d*E
TT    Her    (JD2430000 - 40000) [03504]; since JD2440000 - see Table.
TU    Her    d = 0.022P. P var. Before JD2435000 Min =
TU    Her    2424381.416 + 2.2671303d*E - 854d*10**(-11)*E**2 [09240];
TU    Her    Min = 2437462.3909 + 2.2669718d*E (JD2435000 -
TU    Her    38000) [09241]; Min = 2443324.70097 + 2.2669385d*E
TU    Her    (JD2438000 - 44000) [08593]; since JD2444000 - see Table.
TW    Her    [Fe/H] = -0.47.
TX    Her    Min II 8.97, DII = 0.11P. P var;
TX    Her    periodic term: +0.0081d*sin(0.042deg*(E + 7255)).
UU    Her    [Fe/H] = -1.27.
UU    Her    There was alternation of periods 90d and 71d
UU    Her    [00310]; the period 45d [03507] was also noted.
UU    Her    During JD2443611 - 44161 - see Table. Epoch of Min is given.
UX    Her    Min II 9.11. P var. Before JD2429000 Min =
UX    Her    2419876.467 + 1.5488598d*E [00279]; Min =
UX    Her    2429987.420 + 1.5488513d*E (JD2429000 - 38000)
UX    Her    [03671]; since JD2438000 - see Table.
VW    Her    VB A (B 17.3m, 18", 120deg.
VX    Her    Delta(S) = 5. P var; nonlinear term:
VX    Her    -0.00745d (E:10000)**2. According to [03369],
VX    Her    a member of an eclipsing binary system.
VZ    Her    [Fe/H] = -0.9. P var. P = 0.44031880d (JD2415000 -
VZ    Her    22000) [05738]; Max = 2425004.4590 + 0.44032394d*E
VZ    Her    (JD2422000 - 27000); Max = 2425004.4456 +
VZ    Her    0.44032631d*E (JD2427000 - 36000) [03506];
VZ    Her    since JD2436000 - see Table.
WW    Her    VB A (B 15.6m, 7.4", 148.5deg, white).
WX    Her    Twice longer P is not excluded.
AC    Her    P var.
AC    Her    The Table gives current elements valid since JD2442000.
AC    Her    Mean P = 75.4619d [01754]. The magnitude in
AC    Her    Max varies with Delta(m) = 1.6m [00368].
AD    Her    VB A (B 11.97m, 5", 189deg). d = 0.033P. Min II 9.79.
AF    Her    P var. Before JD2426950 P = 0.630336d;
AF    Her    since JD2426950 - see Table.
AF    Her    The shape of the light curve var.
AG    Her    P var. Max = 2422935.584 + 0.6494378d*E
AG    Her    (JD2418210 - 26952); since JD2426952 - see Table.
AH    Her    Porb = 5.9d:. Oscillations during outbursts:
AH    Her    24s <= P <= 39s, Delta(m) <= 0.003m [09251].
AH    Her    Flicckering in Max And Min up to 0.4m in 2 - 8 minutes
AH    Her    [09252].
AK    Her    ADS 10408 A (B 12.0m, 5", 323deg). Min II 8.64.
AK    Her    Min II - Min I = 0.505P. dII = 0.07P. P var. Before
AK    Her    JD2421200 Min = 2421200.549 + 0.42152207d*E; Min =
AK    Her    2421200.549 + 0.42152083d*E (JD2421200 - 24950);
AK    Her    Min = 2424949.555 + 0.42152061d*E  (JD2424950 -
AK    Her    30000) [01760]; Min = 2430939.368 + 0.42152362d*E
AK    Her    (JD2430000 - 41500); since 2441500 - see Table.
AK    Her    The shape of the light curve var.
AM    Her    3U 1809 +50. Lx(soft)/Lopt ~15.
AM    Her    Emissions of H and KCaII, H, HeI, HeII, etc.
AM    Her    In the spectrum. Epoch of Min I in V light is given.
AM    Her    The period shows complex variations. The phase of Min I
AM    Her    in U light is 0.30p, in B 0.15P, in R 0.05P. Min I is
AM    Her    probably due to an eclipse of a hot spot and the gas flow
AM    Her    near the surface of the white dwarf by the white dwarf
AM    Her    itself. The depth of Min I is up to 0.7m. Min II with the
AM    Her    depth up to 0.4m (sometimes absent), Min II - Min I = 0.55P.
AM    Her    Min II coincides  in phase with the X-ray eclipse.
AM    Her    High and low states (b ~13.0m and B ~15.0m on average);
AM    Her    in the high state there are variations with Delta(m) ~0.3m
AM    Her    on the time scale >= 200d; the duration of low states is
AM    Her    130d - 700d [09258] or less. During low states the
AM    Her    depth of minima is small. Flickering up to 0.8mV in
AM    Her    several minutes or dozens of seconds; X-ray flickering
AM    Her    on the time scale of ~10s not correlating with
AM    Her    optical flickering. The magnetic field ~1*10**7 G at
AM    Her    the equator, ~2*10**7 G on poles. Variable circular
AM    Her    (from  +3% to -9%) and linear (up to 7%) polarization.
AM    Her    IR excess at lambda 10 mkm.
AP    Her    P var strongly. P = 10.400d (JD2415000 -
AP    Her    19000:); P = 10.3970d (JD2423700 - 24700:); P =
AP    Her    10.4260d (JD2424700 - 25300); P = 10.4338D
AP    Her    (JD2425800 - 27000); P = 10.3945d (JD2427000 - 27400);
AP    Her    P = 10.4277d (JD2433000 - 33850); P = 10.3898d
AP    Her    (JD2433850 - 34850);  P = 10.4209d (JD2434850 - 35600);
AP    Her    P = 10.3715d (JD2435600 - 37200);
AP    Her    DURING JD2437200 - 43800 - see Table.
AP    Her    The light curve shape var. [A/H] = -0.8.
AR    Her    P var in a complicated way. Max =
AR    Her    2424794.274 + 0.4700234d*E (1905 - 1954) [06535];
AR    Her    Max = 2439692.683 + 0.469975d*E (1954 - 1967) [05274];
AR    Her    since 1967 - see Table.
AR    Her    Blazhko effect, Pi = 31.5489d [03555],
AR    Her    Delta(m) var (0.9m -: 1.8m pg) [02168], (M - m) var.
AR    Her    Delta(S) = 6.
AT    Her    The star is bright on one plate (JD2418209).
AT    Her    Besides that, 11.8m - 12.25m.
AW    Her    VB A (B 10" - 20"). d = 0.03P.
BB    Her    P var. P = 7.507696D (JD2418924 - 30700);
BB    Her    since JD2430700 - see Table. [A/H] = +0.3.
BC    Her    P var. Before JD2432000 Min = 2426242.372 +
BC    Her    3.08752d*E [09262]; since JD2436000 - see Table.
BD    Her    P var. P = 0.4739135d (JD2426540 - 29620); P =
BD    Her    0.4739057d (JD2429620 - 30570); Max = 2430495.404 +
BD    Her    0.4739126d*E (JD2430570 - before 1948) [09263];
BD    Her    since 1948 - see Table. Delta(S) = 0.8.
BL    Her    P var. P = 1.3074604d (JD2415000 - 35000);
BL    Her    since JD2435000 - see Table. Another possible
BL    Her    representation: Max = 2434999.402 + 1.307457d*E -
BL    Her    3.9d*10**(-10)*E**2 (JD2415000 - 42000). [Fe/H] = 0.0.
BO    Her    d = 0.015P. Min II 10.8. P var?
CC    Her    P var. Min = 2426120.415 + 1.7340314d*E (JD
CC    Her    2425790 - 31265); Min = 2431265.288 + 1.7340460d*E
CC    Her    (JD2431265 - 36000) [02389]; Min = 2439668.342 +
CC    Her    1.73398d*E (JD2436000 - 39600); since JD2439600 - see
CC    Her    Table.
CD    Her    The chart in [06286] is wrong.
CE    Her    [A/H] = -1.8.
CK    Her    P var? Max = 2429231.234 + 0.519201d*E (JD2429231 -
CK    Her    877) [00332]; during JD2436041 - 37955 - see Table.
CO    Her    P2 = 600d. Sometimes does not vary for 150d.
CP    Her    Superimposed waves, 50d - 100d.
CT    Her    The depth of min II 0.05m. P var.
CT    Her    Min = 2430904.431 + 1.786337d*E (JD2426480 - 35000)
CT    Her    [03567]; Min = 2439355.666 + 1.7863645d*E
CT    Her    (JD2435000 - 39500) [00001]; Min = JD2441499.3307 +
CT    Her    1.7863891d*E (JD2439500 - 42500) [08593];
CT    Her    since JD2442500 - see Table.
DE    Her    P var. Max = 2425754 + 171.2d*E (JD2425754 - 30890);
DE    Her    Max = 2430889 + 175.3d*E (JD2430890 - 36150);
DE    Her    during JD2436150 - 38140 - see Table.
DF    Her    Elements are valid since JD2425900.
DH    Her    d = 0.024P:. Min II 9.5.
DI    Her    Min II 8.95, DII = 0.03P, Min II - Min I = 0.77P (1966 -
DI    Her    1978). Apsidal motion: P = 29000yr +- 4000yr;
DI    Her    Min II = 2442241.4602 + 10.5501751d*E.
DI    Her    A considerable discrepancy between the observed and
DI    Her    the theoretical rate of apsidal motion.
DK    Her    P var.
DL    Her    Blazhko effect, Pi = 33.6d, 11.0m <= m Max <= 11.3m. P var.
DL    Her    Delta(S) = 5.
DO    Her    Close to V362 Her.
DQ    Her    VB A (B 18.17m, F, 3.5", 132deg, optical?).
DQ    Her    Nebula, R = 10.5" (Halpha, 1981).
DQ    Her    After the main Max of the Nova a deep
DQ    Her    Min 13.0m (JD2426925) and a flat secondary Max
DQ    Her    6.7m (JD2427065) were observed.
DQ    Her    Eclipsing variability:
DQ    Her    14.61m - 18.08m, Min HeI = 2434954.9445 + 0.193620877d*E
DQ    Her    [09280]. D = 0.20P, d = 0.000P.
DQ    Her    The light curve shape and Delta(M) var.
DQ    Her    Oscillations: Max HeI = JED2434954.785868 +
DQ    Her    8.22521640d*10**(-4)*E - 2.8048d*10**(-16)*E**2
DQ    Her    [08722], 0 <= Delta(m) <= 0.08m.
DQ    Her    Polarization changes with double oscilation period.
DQ    Her    Flickering: Delta(m) = 0.15m.
DY    Her    P var, nonlinear term: -18.6d*10**(-13)*E**2.
EI    Her    Red.
EN    Her    P var. Before JD2427000 P = 160d.
ES    Her    Min II 13.7.
ET    Her    The elements are valid earlier than JD2427200
EX    Her    Red.
EZ    Her    The elements are valid earlier than JD2427400.
FN    Her    P var?
FW    Her    Min II 14.6.
FY    Her    According to the spectrum, EW type is possible.
GL    Her    P var?
GU    Her    d = 0.010P. Min II 11.8. Min II - Min I = 0.513P.
GV    Her    [Fe/H] = -1.41. P var. Max = 2427543.360 +
GV    Her    0.2914606d*E (JD2427543 - 29728) [00152];
GV    Her    during JD2436041 - 38170 - see Table.
GY    Her    P var. Max = 2428219.623 + 0.524347d*E (JD2428219 -
GY    Her    727) [00152]; during JD2436370 - 38170 - see Table.
HS    Her    d = 0.025P. Min II 8.63. P var; since JD2438240 - see
HS    Her    Table. Apsidal motion: Pi ~130yr [06538].
HV    Her    d = 0.008P:; Min II 12.9:.
HZ    Her    Her X-1 = 4U 1656 + 35. Lx/Lopt = 2 - 60.
HZ    Her    The Table gives elements for light minima due
HZ    Her    to eclipsing variability and the reflection effect. Min I
HZ    Her    coincides with the X-ray eclipse. Shallow Min II may
HZ    Her    be present. The reflection effect causes variations
HZ    Her    with Delta(m) up to 1.5m. A cycle of 34.875d duration is
HZ    Her    observed in X-ray band; the source is faint during
HZ    Her    two thirds of the cycle. The optical light curve changes
HZ    Her    are observed during the 35d cycle [09283]. According to
HZ    Her    [06539], during JD2427543 - 657 and JD2428630 - 29789 the
HZ    Her    strong reflection effect was absent; the star was still
HZ    Her    varying with P = 1.7d and had Delta(m) ~0.5m,
HZ    Her    Min I = Min II. In [06546] it is stated that
HZ    Her    such intervals with no reflection effect, of 8d to 7a
HZ    Her    duration, took place for almost half the time since
HZ    Her    1890. The light changes during such intervals are in
HZ    Her    the range 14.7m - 15.2m pg. Since 1957 intervals without
HZ    Her    the reflection effect were not observed. In June - July
HZ    Her    1983 the predicted phases of high X-ray flux
HZ    Her    did not take place, but the reflection effect did not
HZ    Her    disappear [09284]. Secondary light variations: P1 =
HZ    Her    1.0977d (delta(B1) = 0.33m), P2 = 0.871173d*E
HZ    Her    (delta(B2) = 0.10m),
HZ    Her    P3 = 1.623846d*E (delta(B3) = 0.17m) [09285]. X-ray pulsar,
HZ    Her    P = 1.2377991s (JD2443357), dP/dt/P = (-2.9 +- 0.2)*10**(-6)/yr
HZ    Her    [09286], sometimes noticeable also in the
HZ    Her    optical range [06543]. Rapid brightness flickering.
IK    Her    d = 0.030P?
IQ    Her    Superposition of variations with shorter P and
IQ    Her    small Delta(m) [06645].
IT    Her    According to the spectrum, EW type is possible.
KL    Her    Min II 14.7.
KV    Her    The light curve is characteristic of Mira Ceti stars
KV    Her    but strongly varies. Many irregularities. O - C: -96d, +73d.
LR    Her    Min II 15.4:.
LS    Her    The light curve shape var.
LT    Her    d = 0.02P. Min II 10.79.
LV    Her    P var? During JD2428429 - 31342 - see Table.
MM    Her    VB A (B 13.50m, 18", 120deg). Min II 9.7.
MM    Her    Delta(m) of the distorsion wave up to 0.12m.
MP    Her    [Fe/H] = -1.18.
MS    Her    Min II 13.3.
MT    Her    Min II 12.30.
MV    Her    The chart in [00156] identifies the variable erroneously;
MV    Her    real MV Her is marked as "C".
MW    Her    P var. P = 503d (1976) [09290]. During
MW    Her    JD24668 - 29172 - see Table.
MX    Her    Moments of Min after JD2444000 published by different
MX    Her    groups of observers contradict each other.
NQ    Her    According to [03882], EA, 8.0 - 8.6 pg, Min II
NQ    Her    8.4, Min I = 2426894.433 + 0.870218d*E (JD2426894 - 34250).
NR    Her    Waves, P = 2.8d - 5.5d.
OQ    Her    Epoch of min is given.
OS    Her    B - V: +0.12,  +0.48.
OU    Her    Spectral type is given according to [02198]; in BSD-G7.
OX    Her    Delta(S) = 6:.
PW    Her    Min II 10.1; DII ~0.3P(!).
V0338 Her    Min II 10.13. P var. Before JD2437000 Min =
V0338 Her    2433771.38 + 1.305732d*E [03115]; Min = 2441864.379 +
V0338 Her    1.3057515d*E (JD2437000 - 43400) [08593, 00001];
V0338 Her    since JD2443400 - see Table.
V0342 Her    Min II 10.7.
V0347 Her    P var. Max = 2415288.21 + 0.5373619d*E (JD2415288 -
V0347 Her    18596); since JD2429495 - see Table.
V0359 Her    P var. Min = 2416046.476 + 1.755754d*E (JD2416000 -
V0359 Her    26500) [00001]; Min = 2435693.47 + 1.755775d*E (JD
V0359 Her    2426500 - 36000) [01040]; since JD2443500 - see Table.
V0362 Her    Close to DO Her.
V0365 Her    Blazhko effect: Pi = 40.64d. P var.
V0365 Her    During JD2429037 - 36840 - see Table.
V0373 Her    P = 0.33d or 0.50d is possible.
V0384 Her    P ~0.33d is possible.
V0387 Her    Min II 13.2.
V0394 Her    P var?
V0395 Her    Z = 0.0643.
V0396 Her    Z = 0.175.
V0403 Her    Min II 16.0:.
V0412 Her    Min II 15.2.
V0422 Her    P var? During JD2434131 - 35991 - see Table.
V0423 Her    Min II 15.0.
V0426 Her    Min II 15.8.
V0431 Her    P var.
V0436 Her    The elements are uncertain.
V0441 Her    IR excess, evidence for a circumstellar envelope. Possibly
V0441 Her    non-radial pulsation.
V0442 Her    P var. Max = 2434223.375 + 0.4421143d*E (JD2417447 - 36083);
V0442 Her    since JD2435730 - see Table.
V0442 Her    The shape of the light curve varies.
V0446 Her    Before the outburst 16.2m - 18.8m [03607].
V0451 Her    ADS 10310 A (B 10.70m, 19", 239deg).
V0451 Her    The epoch of Min U light is given.
V0458 Her    [Fe/H] = -1.65.
V0463 Her    P = 54.4d is possible.
V0477 Her    Min II 15.4.
V0482 Her    Possibly eclipsing.
V0499 Her    Blazhko effect.
V0502 Her    Min II 13.5?
V0510 Her    P var?
V0511 Her    P var?
V0513 Her    Min II 15.7.
V0516 Her    Min II 17.1.
V0523 Her    Elements are valid during JD2430940 - 990.
V0524 Her    Twice shorter P is possible.
V0527 Her    Max = 2430938.451 + 0.5188d*E (JD2430938 - 990);
V0527 Her    during JD2436308 - 318 - see Table.
V0529 Her    Epoch of Min is given.
V0529 Her    According to [04217], P = 120d.
V0533 Her    VB A (B 16m, 9.5", 0deg). oscillations:
V0533 Her    Max = 2443717.730281 + 0.0007364941d*E, A ~1% [04162].
V0551 Her    P = 4.00d/n is possible.
V0552 Her    P = 3.04d/n is possible.
V0554 Her    P = 4.01d/n is possible.
V0557 Her    P = 8.00d/n is possible.
V0570 Her    P = 0.5d or 0.33d is possible.
V0578 Her    Red.
V0581 Her    Several close companion.
V0582 Her    VB. Red.
V0583 Her    Red.
V0588 Her    Possibly eclipsing.
V0600 Her    SB, Porb - see Table. Variability of Vr possibly caused by
V0600 Her    BCEP type pulsations: P - 0.18d.
V0601 Her    Elements are valid since JD2439184.
V0604 Her    Red.
V0608 Her    Blazhko effect.
V0615 Her    Red.
V0618 Her    P var?
V0624 Her    VB A (12.04m, 40"). Min II 6.35. SB2.
V0637 Her    ADS 10227 A (BC 9.2m, 9.2m, 1.7", 18deg, 1975; BC: A =
V0637 Her    0.28", Porb = 56.56yr).
V0639 Her    mu alpha = -0.21", mu delta = +0.39",pi = 0.087".
V0639 Her    VB B (A = V647 Her, 11.36m var, dM4e; B 16", 268deg).
V0639 Her    Flares in the bands U and M pg.
V0640 Her    VB A (B 14.9m, 8.5", 217deg; C 13.9m, 23", 221deg).
V0641 Her    L or ISB type is also possible.
V0644 Her    SB (Porb = 11.859d).
V0645 Her    P ~3h - 10h, a cycle of 40d.
V0647 Her    VB A (B = V639 Her, 16", 268deg); mu alpha = -0.21",
V0647 Her    mu delta = +0.39"; pi = 0.087".
V0652 Her    P var; nonlinear term: -45.80d*10**(-10)*E**2. Delta(m) var.
V0652 Her    Resembles PV TEL type stars but is a helium rich subdwarf.
V0652 Her    Epoch of Max is given. Secondary hump at the phase 0.5P.
V0654 Her    Delta(m) = 0.15m in white light.
V0655 Her    ADS 10407 A (B 9.2m, 4.1", 144deg, 1971).
V0657 Her    According to [02610], CST?, 11.0m.
V0662 Her    Less probable P values: 0.56629d, 0.56710d, 0.56881d,
V0662 Her    0.56970d.
V0685 Her    Min II 15.8.
V0687 Her    Min II 14.9.
V0691 Her    Possible P values: 0.927d, 0.637d.
V0697 Her    H2O, OH maser.
V0699 Her    Min II 16.0:.
V0717 Her    Blazhko effect?
V0718 Her    Min II 14.3.
V0719 Her    EW type with twice longer P is not excluded.
V0720 Her    Blazhko effect?
V0721 Her    Blazhko effect?
V0722 Her    Min II 15.7.
V0723 Her    Min II 15.5.
V0728 Her    Min II 11.4.
V0731 Her    Min II 13.8.
V0731 Her    Twice shorter P is not excluded.
V0732 Her    Min II 13.8.
V0733 Her    Min II 14.3:.
V0737 Her    Blazhko effect?
V0740 Her    Min II 14.4.
V0741 Her    Blazhko effect?
V0742 Her    Min II 14.4.
V0744 Her    Vr var, P = 86.7221d (SB1? nonradial pulsatiob?).
V0744 Her    Rapid spectral variability is possible: P = 2.5552d,
V0744 Her    0.78906d.
V0749 Her    P = 465s.
V0771 Her    Epoch of max U light is given.
V0772 Her    VB AB (7.4m, G0V; 8.5m, G8V:; A = 0.27", E = 0.97, P =
V0772 Her    20.0yr, C 10.62m, 28"). One of the components
V0772 Her    (probably B) is SB1, P = 0.879511d [04056]. The same
V0772 Her    component must be the eclipsing system. Faint X-ray
V0772 Her    source.
V0774 Her    Both flares and "antiflares" (abrupt fadings) of
V0774 Her    comparable amplitude are observed.
V0946 Her    Not Wolf 688, a large-proper-motion star, which is at 17h19m28s.9,
V0946 Her    +33deg05'10" (epoch and equinox 2000.0).
V0973 Her    Suspected rapid brightness variations.
V0994 Her    The secondary component of the double system may also vary.
V1088 Her    MinII 14.1.
V1091 Her    MinII 12.27.
V1092 Her    The depth of MinII is 0.46. VB B (B GSC 02073-00504, 14").
V1093 Her    Multi-mode pulsations at a time scale of hours.
V1094 Her    MinII 13.08.
V1095 Her    MinII 12.40.
V1099 Her    Multi-mode pulsations of an sdB star at a time scale of hours.
V1101 Her    MinII 12.47.
V1102 Her    MinII 14.27.
V1103 Her    MinII 12.37.
V1106 Her    MinII 12.9. DSCT type with a twice shorter period is also possible [264, 040].
V1108 Her    VB B (A 1" sf). The finding chart in [247] is incorrect.
V1117 Her    Flat waves near maximum and deep fadings. IR excess.
V1124 Her    Blazhko effect? P(Bl) = 38.4d:. A pulsation period of 0.3551d is not excluded.
V1131 Her    The tabulated amplitude can be too low because of a neighboring star.
V1135 Her    According to [007], besides eclipses with P = 39.7d, the star is pulsating with P2 = 4.23d.
V1137 Her    Min II = 14.7.
V1138 Her    Min II = 14.0.
V1140 Her    Min II = 14.1.
V1141 Her    Multiperiodic, three close, nearly equidistant frequencies. P1 is tabulated (semi-amplitude 0.105m); P2 = 0.320340d (0.053m); P3 = 0.314355d (0.040m).
V1143 Her    Min II = 11.7.
V1144 Her    Min II = 15.4 :.
V1146 Her    Min II = 11.45:.
V1158 Her    Type RRC with a twice shorter period is possible.
V1211 Her    Multiperiodic.
V1227 Her    Porb = 0.06319d.
V1231 Her    VB A (B 12.9mV, 12", 289deg, 1999).
V1236 Her    VB AB (10.2m, 11.2m, 1.3", 331deg, 2009).
V1239 Her    Eclipsing variability in quiescence: 17.4m - 19.1mV, Min = 2453648.236507 + 0.10008215d x E, D = 0.1P.
V1250 Her    Ultraviolet flare amplitude in excess of 1.4m.
V1265 Her    Blazhko effect?
V1285 Her    The elements tabulated are for the first overtone. P0 = 0.5539d.
V1290 Her    SB1, Porb = 45.6228d.
V1299 Her    Type SRB is not excluded.
V1302 Her    VB B (A 12.2mV; B 12.4mV, 13", 266deg, 1998).
V1304 Her    VB A (B 12.1m, 16", 329deg, 2000).
V1314 Her    Blazhko effect?
V1323 Her    Intermediate polar; variations with only the spin period were detected. Porb = 0.11126d.
V1344 Her    MinII - MinI = 0.545P.
alf   Her    ADS 10418 A (B 5.39m, 4.9", 107deg, 1973; B - SB2,
alf   Her    G5III + F2V). Slow variations, P ~6yr, Delta(m) ~0.5m;
alf   Her    quicker changes, P ~ 50d - 155d, Delta(m) ~ 0.3m - 1.0m.
alf   Her    Together with the visual companion the
alf   Her    star is surrounded by an enormous envelope (R ~2*10**5R$,
alf   Her    expansion velocity 10 km/s, mass loss 3*10**(-8)M$/yr).
nu.   Her    [Fe/H] = -0.26. SB?
omi   Her    VB interferometric.
phi   Her    SB, Porb = 560.5d.
ome   Her    ADS 10054 A (B 11.5m, 0.8", 232deg, 1967; C 11.0m, 28.4",
ome   Her    96deg, 1957; D 27.5", 271deg, 1960). Epoch of Min is given.
ome   Her    Double wave in the light curve.
ome   Her    Rapid variations, P = 0.15d [09310].
g     Her    The mean cycle 1972 - 1981 is given. Slow pulsations
g     Her    (P = 875d +- 70d) and non-periodic variations on the
g     Her    time scale of 5d - 15d with Delta(m) up to 0.2m are
g     Her    superimposed.
u.    Her    ADS 10449 A (B 10.2m, 4.4", 60deg). Min II 4.93.
R     Hor    OH, H2O, SiO maser. P var. Max = 2428868 + 401.5d*E
R     Hor    (JD2412800 - 28900); since JD2428900 - see Table.
V     Hor    P = 59d (JD2428380 - 910), P = 90d (JD2429170 - 980).
X     Hor    Epoch of Min brightness is given. Maxima are broad.
X     Hor    Usually secondary minima are observed.
SY    Hor    Min II 12.0.
SZ    Hor    Min II 10.7:.
TU    Hor    Min II 6.03; Min II - Min I = 0.52P;
TU    Hor    Max II is fainter than Max I by 0.05m. Peculiar
TU    Hor    ellipsoidal variable [09245].
TY    Hor    Type RCB?
UU    Hor    P var. Max = 2416826.417 + 0.6436900d*E (JD2416800 - 25000);
UU    Hor    since JD2425000 - see Table.
UX    Hor    Min II 14.4. P var. Min I = 2426659.380 + 0.7126943d*E
UX    Hor    (JD2426650 - 30860); since JD2430540 - see Table.
UZ    Hor    P var. Max = 2426679.425 + 0.338188d*E (JD2426300 - 28430);
UZ    Hor    since JD2430040 - see Table.
VY    Hor    mu = 0.173", ro = 33deg. P = 314s, 617s.
R     Hya    VB A (B 13.0m, 21.6", 324deg). SiO maser. P var. According
R     Hya    to [00458]; Max = 2328201 + 486d*E (JD2328200 - 31120);
R     Hya    Max = 2343512 + 507d*E (JD2343300 - 44800);
R     Hya    Max = 2372678 + 485d*E (JD2372200 - 72700);
R     Hya    Max = 2380447 + 477d*E (JD2380000 - 81400);
R     Hya    Max = 2385160 + 461d*E (JD2384700 - 88000);
R     Hya    Max = 2394350 + 448.6d*E (JD2393900 - 2402000);
R     Hya    Max = 2403742 + 434d*E (JD2403300 - 04200);
R     Hya    Max = 2406363 + 429.5d*E (JD2406000 - 11100);
R     Hya    Max = 2413642 + 411d*E (JD2413200 - 14100);
R     Hya    Max = 2416563 + 405.5d*E (JD2416100 - 23400);
R     Hya    Max = 2424288 + 414.7d*E (JD2423400 - 28500).
R     Hya    since JD2428500 - see Table.
T     Hya    P var. Max = 2399455 + 289.00d*E(JD2398600 - 2421700);
T     Hya    Max = 2422584 + 294.2d*E (JD2421700 - 25800);
T     Hya    Max = 2431781 + 284.20d*E (JD2425800 - 36200); since
T     Hya    JD2437500 - see Table.
V     Hya    VB A (B 11.58mV, KO III, 46", 186deg).
V     Hya    Mean brightness variations with P = 6670d and A = 3.5m are
V     Hya    superimposed by light oscillations with A = 1.1m - 2m and
V     Hya    elements given in the Table. Deep light minima were
V     Hya    observed in 1891, 1908, 1925, 1942 - 43, 1959,  and 1962.
V     Hya    A graph of the light curve [03614].
W     Hya    VB A (B 9.3m, 72", 108deg). P var. Max = 2411074 + 379d*E
W     Hya    (JD2411000 - 14150); Max = 2414644 + 395d*E
W     Hya    (JD2414150 - 19400); Max = 2419746 + 378d*E
W     Hya    (JD2419400 - 25200) [00458]. Max = 2425740 + 366d*E
W     Hya    (JD2425200 - 27000); Max = 2440336 + 397.35d*E
W     Hya    (JD2428000 - 40500); since JD2440500 - see Table.
W     Hya    Amplitude and shape of the light curve vary strongly.
W     Hya    OH, H2O, SiO maser.
X     Hya    OH, H2O, SiO maser.
Y     Hya    Mean magnitude varies.
RR    Hya    H2O maser.
RS    Hya    P var. Max = 2422973 + 330.2d*E (JD2414000 - 23000);
RS    Hya    Max = 2429126 + 342.0d*E (JD2423000 - 29200); Max =
RS    Hya    2429455 + 331.2d*E (JD2429200 - 34500);
RS    Hya    since JD2434500 - see Table.
RT    Hya    Before 1952 P = 255d; since 1952 - see Table.
RT    Hya    The character And amplitude of light variations vary
RT    Hya    strongly.
RU    Hya    OH, H2O maser. P var. Max = 2429572 +
RU    Hya    334.0d*E (JD2414000 - 29600); since JD2428500 - see
RU    Hya    Table.
RW    Hya    SB2 (P = 370d). Epoch of Min brightness is given.
RX    Hya    VB A (B 10.5m). Depth of Min II 0.05m. P var.
RX    Hya    Min I = 2428261.385 + 2.2815942d*E (JD2419500 -
RX    Hya    28500); Min I = 2440650.409 + 2.2816200d*E
RX    Hya    (JD2428500 - 41400); since JD2441400 - see Table.
SS    Hya    VB A (B 12.0m, 13", 195deg); SB2.
SU    Hya    Mean magnitude varies with P = 780d.
SV    Hya    VB A (B 35", 225deg). Delta(S) = 7.
SX    Hya    D = 0.022P. P var. Min I = 2427659.223 + 2.895697d*E
SX    Hya    (JD2410000 - 28000) [00007]; since JD2442500 - see Table.
SY    Hya    P var. Min = 2425590.589 + 3.403082d*E (JD2425500 -
SY    Hya    31150) [07548]. Since JD2432200 - see Table.
SZ    Hya    P var. Max = 2415714.1429 + 0.53742815d*E
SZ    Hya    (JD2414700 - 26500) [03626]; Max = 2426410.575 + 0.53736d*E
SZ    Hya    (JD2426400 - 27200) [00001]; Max = 2431881.5537 +
SZ    Hya    0.53723051d*E (JD2427880 - 35200) [03626]; Max =
SZ    Hya    2435542.267 + 0.5372497d*E (JD2435500 - 38900)
SZ    Hya    [03627]. Since JD2438770 - see Table.
SZ    Hya    Blazhko effect: Max(A) = 2440705 + 25.8d*n [06557];
SZ    Hya    10.44m <= Max <= 11.03m.
TT    Hya    Min II 7.32; d = 0.035P.
TU    Hya    P var. Max = 2416980 + 277.5d*E (JD2412500 -
TU    Hya    17300); Max = 2417260 + 272.5d*E (JD2417200 -
TU    Hya    19800) [01787]; Max = 2430410 + 281.4d*E
TU    Hya    (JD2420500 - 30500); Max = 2438332 + 272.3d*E
TU    Hya    (JD2432000 - 39200); since JD2439200 - see Table.
TY    Hya    P var. Min = 2434478.464 + 4.660978d*E (JD2419800 -
TY    Hya    35000) [01788]; since JD2435000 - see Table.
UU    Hya    P var. Max = 2427423.84 + 0.5238585d*E (JD2414950 - 27400)
UU    Hya    [01789]; Max = 2429729.835 + 0.523854d*E (JD2427000 - 31000)
UU    Hya    [00752]. Spectrum is based on Ca II.
UW    Hya    Min II 13.8:; Min II - Min I = 0.64P. P = 1.055439d?
UY    Hya    Min II 13.8. RRC?
VV    Hya    P var. Max = 2427421 + 155d*E (JD2419500 - 37000)
VV    Hya    [01792]; since JD2437000 - see Table.
VX    Hya    (k - b)2 = 0.26.
VX    Hya    Luminosity class [03149] contradicts the type of light
VX    Hya    variability. The shape of the light curve strongly varies.
VX    Hya    The main oscillation with the period P0 given in the Table
VX    Hya    is superimposed by the secondary one with P1 = 0.172720d
VX    Hya    [03631]. P1/P0 = 0.773; Pb = 0.761445d.
VY    Hya    Min II 9.1.
VZ    Hya    Min II 9.46.
WY    Hya    Min II 11.2.
WZ    Hya    (k - b)2 = 0.06. P var. Max = 2416169.681 + 0.53772640d*E
WZ    Hya    (JD2414000 - 19000); Max = 2419811.736 +
WZ    Hya     + 0.53775858d*E (JD2419000 - 21000); Max =
WZ    Hya     = 2424618.630 + 0.53774101d*E (JD2421000 - 32000)
WZ    Hya    [00752]; Max = 2436613.445 + 0.5377229d*E
WZ    Hya    (JD2436600 - 38500) [03633]; since JD2438000 - see Table.
XX    Hya    P var. Max = 2439560.355 + 0.50774868d*E
XX    Hya    (JD2428200 - 39560) [05238]; since JD2439560 - see Table.
XZ    Hya    Min II 15.0.
AE    Hya    Min II 14.6.
AF    Hya    Min II 13.8.
AI    Hya    Min II 9.84; Min II - Min I = 0.438P; DII = 0.075P;
AI    Hya    dI = 0.02P; dII = 0.00P; EA/DM. Pulsation
AI    Hya    period P' = 0.13803d, A = 0.02m - 0.03m [09259].
AV    Hya    Min II 10.35; dI = 0.023P:.
CH    Hya    Min II 15.5; Min II - Min I = 0.57P.
CO    Hya    Found in Centaurus, in 10deg to the south from the position
CO    Hya    published by the discoverer [00078].
CW    Hya    P var? [04027].
CW    Hya    Elements given in the Table satisfy observations only in
CW    Hya    the interval JD2428950 - 30375.
DD    Hya    P var. Max = 2431139.313 + 0.501818d*E (JD2431100 -
DD    Hya    600) [01432]. Since JD2441600 - see Table.
DE    Hya    d = 0.014P?
DF    Hya    Min II 11.5.
DH    Hya    Delta(S) = 7.
DK    Hya    Min II 10.7.
DM    Hya    d = 0.15P?
EU    Hya    Min II 10.2.
EX    Hya    Light variations with Porb and amplitude up to 0.9mV
EX    Hya    due to eclipses of hot spot are represented by the
EX    Hya    elements: ET(Min) = 2437699.94177 + 0.0682338422d*E,
EX    Hya    where ET(Min) is the heliocentric Julian Date converted
EX    Hya    to Ephemeris Time; simultaneously periodic modulation of
EX    Hya    the shape of the light curve between the outbursts is
EX    Hya    observed with the amplitude 0.2m - 0.9m and the elements:
EX    Hya    Max = 2437699.8895 + 0.04654656d*E - 1.2d*10**(-12)*E**2
EX    Hya    [09265]. Mean interval between bright outbursts is 465d
EX    Hya    [05695], mean cycle is close to 20 - 30d.
EY    Hya    P var. Max = 2432707 + 160.5d*E (JD2426100 - 32800);
EY    Hya    since JD2432800 - see Table.
EZ    Hya    Min II 10.7. P var. Min I = 2440255.8482 + 0.44976658d*E
EZ    Hya    (JD2431160 - 40650) [07549]; since JD2440250 - see Table.
FG    Hya    Min II 10.25; dI = dII = 0.085P. P var. Min I =
FG    Hya    2431150.388 + 0.3278422d*E (JD2431140 - 34400)
FG    Hya    [00182]; Min I = 2436968.7067 + 0.32783433d*E
FG    Hya    (JD2434050 - 400) [03639]; Min I = 2436968.7067 +
FG    Hya    0.32783546d*E (JD2436950 - 43250) [09267];
FG    Hya    since JD2444600 - see Table.
FI    Hya    V27 in the globular cluster NGC 4590
FI    Hya    (M68); cluster non-member.
FS    Hya    According to [01480] P = 91.7d.
FW    Hya    Min II 12.4.
FY    Hya    VB A (B 15.45m, 15", 90deg); Delta(S) = 7:; (k - b)2 = -0.03.
GK    Hya    Min II 9.57.
GK    Hya    There is a square term in the elements:
GK    Hya    -4.01d*10**(-9)*E**2.
GM    Hya    d <= 0.01P.
GN    Hya    Min II 13.6.
GT    Hya    Cep?
HS    Hya    Min II 8.55.
IK    Hya    Blazhko effect with Pi ~30d.
IW    Hya    OH, H2O maser.
KM    Hya    P var?
KU    Hya    VB AB (7.3m, 7.4m, A = 0.150", P = 58.93 yr, E = 0.219);
KU    Hya    A(v) = 0.06m.
KW    Hya    Porb = 7.75043d; E = 0.110 [09273]; Min II 6.35;
KW    Hya    Min II - Min I = 0.54P.
V0404 Hya    MinII 15.10.
V0412 Hya    MinII 12.9:.
V0420 Hya    Porb = 764 d. Symbiotic features in the spectrum.
V0421 Hya    Variable brown dwarf.
V0427 Hya    VB A (B 13.9mpg, 22", 305deg, 1999; C 14.8mpg, 35", 276deg, 1999).
V0430 Hya    Blazhko effect?
V0434 Hya    MinII - MinI = 0.54P.
V0443 Hya    A twice shorter period is not excluded.
V0453 Hya    A twice shorter period is not excluded.
V0466 Hya    Min II = 11.6. O'Connell effect.
V0468 Hya    P varies? [001].
V0470 Hya    Min II = 13.50.
V0472 Hya    Min II = 12.5.
V0474 Hya    Min II = 12.2.
V0475 Hya    Min II = 13.2.
V0476 Hya    Min II = 13.1.
V0477 Hya    Min II = 16.2.
V0483 Hya    Min II = 12.55.
V0484 Hya    A brown dwarf with periodic brightness variations.
V0488 Hya    A brown dwarf with periodic brightness variations.
V0490 Hya    Min II = 8.71:. VB AB (8.81m, 10.93m, 1".10, 169deg, 1991).
V0498 Hya    Superhumps: P = 0.06036d.
V0500 Hya    P1 is tabulated; P0 = 0.56391d. Amplitude ratio A1/A0 = 2.45.
V0502 Hya    Min II = 10.09. VB AB (A 10.3m var; B 12.3m, 2.2", 72deg, 1943).
V0504 Hya    Type EW with a twice longer period is possible.
V0511 Hya    Min II = 9.05.
V0514 Hya    Min II = 14.5:.
V0515 Hya    P = 0.269198d is also possible.
V0518 Hya    The star's position coincides with SN 2001am.
V0519 Hya    Min II = 12.50.
V0520 Hya    P = 0.331234d is also possible.
V0522 Hya    P = 0.255132 is also possible.
V0524 Hya    Min II = 17.6.
V0541 Hya    Multiperiodic.
V0542 Hya    Min II = 10.40. dP/dt = -0.45 x 10^(-5) d/yr. VB AB (10.8m, 11.7m, 2", 42deg, 2003).
V0543 Hya    Blazhko effect, P = 59d.
V0545 Hya    Min II = 11.98. Besides variations with the tabulated period, a second EW periodicity is revealed, P2 = 0.353901d, with amplitudes of both minima about 0.25m.
V0547 Hya    VB A (B = V0548 Hya, 5", 148deg, 1999).
V0548 Hya    VB B (A = V0547 Hya; AB 5", 148deg, 1999).
V0549 Hya    VB B (A = V0550 Hya; AB 13", 185deg, 2000).
V0550 Hya    VB A (B = V0549 Hya, 13", 185deg, 2000).
V0551 Hya    Multiperiodic.
V0552 Hya    Blazhko effect, P = 48.3d.
V0553 Hya    Min II = 12.90.
V0554 Hya    Min II = 13.2.
V0555 Hya    Min II = 12.20.
V0559 Hya    Blazhko effect, P = 26.50d.
bet   Hya    VB A (B 5.6m, 0.9", 8deg, 1959).
khi 2 Hya    Min II 5.92.
Y     Hyi    d = 0.024P.
RS    Hyi    In the region of the Small Magellanic Cloud.
RS    Hyi    Not a member of the cloud.
RT    Hyi    Min II 14.1.
RV    Hyi    Min II 12.4; Min II - Min I = 0.61P.
RY    Hyi    In the region of the Small Magellanic Cloud. Not a member
RY    Hyi    of the Cloud.
ST    Hyi    The member of the Small Magellanic Cloud. [A/H] = -0.8.
SZ    Hyi    In the region of the Small Magellanic Cloud. Not a member
SZ    Hyi    of the Cloud.
TW    Hyi    Delta(S) = 10:.
UU    Hyi    P = 112.25d?
VW    Hyi    Mean interval between the supermaxima is 179d.
VW    Hyi    Porb = 0.0742711d. Between the normal outbursts the
VW    Hyi    brightness periodically increases by 0.35m - 0.40m because
VW    Hyi    of hot spot appearances:
VW    Hyi    Max = 2440128.0222 + 0.0742711d*E [07550]. During the
VW    Hyi    supermaxima the period between the superhumps is
VW    Hyi    0.0769d [09275]. Sometimes the light oscillations with
VW    Hyi    the amplitude 2% and cycle from 28s to 34s are observed
VW    Hyi    [07551].
VY    Hyi    In the region of the Small Magellanic Cloud. Not a member
VY    Hyi    of the Cloud.
VZ    Hyi    RR [00193].
WX    Hyi    Mean interval between the supermaxima is 141.5d.
WX    Hyi    Porb = 0.0748134d [09277]. Period between the superhumps
WX    Hyi    observed during the supermaxima is 0.07737d [09278].
WZ    Hyi    In the region of the Small Magellanic Cloud. Not a member
WZ    Hyi    of the Cloud.
ZZ    Hyi    A galaxy PGC 232232 [00001].
AC    Hyi    In the region of the Small Magellanic Cloud. Not a member
AC    Hyi    of the Cloud.
BB    Hyi    Delta(S) = 7:.
CY    Hyi    MinII 9.8.
DM    Hyi    Type RR with P = 0.64272d or 0.39125d is also possible.
V     Ind    P var. Max = 2439792.276 + 0.4796030d*E
V     Ind    (JD2414000 - 40000) [05233]; since JD2440000 - see Table.
V     Ind    Delta(S) = 7, (k - b)2 = 0.02.
RS    Ind    Min II 10.0. P var.
RU    Ind    VB A (B 12.6m, 2.3", 103deg). Min II 12.1.
RX    Ind    240d < P < 310d.
RY    Ind    Min II 11.04.
ST    Ind    Min II 11.79.
SU    Ind    Min II 9.5:.
TV    Ind    Min II 11.9.
AR    Ind    Min II 14.4. RRC?
AY    Ind    mu alpha =  +0.345", mu delta = -0.310"; VB?
CH    Ind    MinII 8.14:.
CI    Ind    A variable double brown dwarf. VB (0.7").
CK    Ind    Besides 6 Gamma Dor modes, a Delta Sct mode (P = 0.039 d) was detected.
CQ    Ind    MinII - MinI = 0.33P.
CZ    Ind    Blazhko effect, P = 133d.
R     Lac    VB A (B 14.1m, 6", 50deg).
S     Lac    P var. Max = 2412857 + 238.2d*E (JD2410000 - 16400);
S     Lac    Max = 2418828 + 241.45d*E (JD2416400 - 20500); Max =
S     Lac    2427307 + 242.7d*E (JD2420500 - 27300); Max =
S     Lac    2437290 + 237.4d*E (JD2427300 - 37300);
S     Lac    since JD2437300 - see Table.
U     Lac    There are light variations with the periods:
U     Lac    150d, 550 - 690d, 2900d.
V     Lac    P var. There is a square term in the elements:
V     Lac    -6.48d*10**(-8)*E**2.
W     Lac    P var. Max = 2415255 + 323d*E (JD2414600 - 15300);
W     Lac    Max = 2425628 + 335.5d*E (JD2425600 - 38000) [00458];
W     Lac    Max = 2433844 + 324.5d*E (JD2428000 - 33850);
W     Lac    since JD2433850 - see Table.
X     Lac    P var. Max = 2418890.497 + 5.444303d*E (JD2416670 -
X     Lac    29500) [02033]; since JD2429500 - see Table.
Z     Lac    P var. There is a square term in the elements:
Z     Lac    -3.4d*10**(-8)*E**2. [A/H] = 0.2.
RR    Lac    P var. Max = 2419434.331 + 6.416146d*E (JD2417900 - 31600);
RR    Lac    since JD2431600 - see Table. [A/H] = 0.0.
RT    Lac    Min II 9.62. P var. Min I = 2440382.9005 + 5.0740484d*E +
RT    Lac    1.02d*10**(-8)*E**2 (JD2411650 - 42500) [08592];
RT    Lac    since JD2436470 - see Table.
RT    Lac    There is a square term in the elements given in the Table:
RT    Lac    -2.7d*10**(-8)*E**2. Shape of the light
RT    Lac    curve and depths of the Minima vary. According to
RT    Lac    [09293] the period of the distortion wave migration is
RT    Lac    ~9.5 yr, the period of the wave amplitude variations
RT    Lac    (0 < A <= 0.17m) is ~30 yr. According to [09292] the
RT    Lac    migration period is nearly half of the value given in
RT    Lac    [09293].
RV    Lac    Mean magnitude varies with the period 550 - 700d.
RW    Lac    Min II 10.8; DII = 0.024P; Min II - Min I = 0.492P.
RX    Lac    S7.5/1e. P = 174d (JD2414950 - 29550) [01026];
RX    Lac    since JD2436800 - see Table.
RY    Lac    Oscillations of mean magnitude with P = 300 - 420d
RY    Lac    and A <= 0.5m are superimposed by oscillations with
RY    Lac    P = 38 - 91d.
SS    Lac    Probable member of the open cluster NGC 7209. Min II 10.5;
SS    Lac    Min II - Min I = 0.57P; d = 0.008P.
SS    Lac    Apsidal motion with P = 1000 yr is possible.
ST    Lac    Elements should be checked.
SU    Lac    P var. Max = 2412748 + 279.10d*E (JD2412700 - 27000)
SU    Lac    [05707]; Max = 2426972 + 286.74d*E (JD2426900 - 31000);
SU    Lac    Max = 2431008 + 306.0d*E (JD2431000 - 33150)
SU    Lac    [00001]; Max = 2433150 + 319.14d*E (JD2433150 - 42150)
SU    Lac    [05707]; since JD2442100 - see Table.
SW    Lac    Min II 9.31. P var. Min I = 2418943.712 + 0.32071236d*E
SW    Lac    (JD2410000 - 19990); Min I = 2420038.621 +
SW    Lac    0.32071510d*E (JD2419990 - 25210); Min I =
SW    Lac    2430996.525 + 0.32071665d*E (JD2425210 - 33690);
SW    Lac    Min I = 2436046.5634 + 0.32072132d*E (JD2433690 - 36755)
SW    Lac    [05222]; Min I = 2437572.5723 + 0.32072811d*E
SW    Lac    (JD2436755 - 40000) [03374]; Min I = 2440467.4592 +
SW    Lac    0.32072480d*E (JD2440110 - 40500) [06089]; Min I =
SW    Lac    2441249.3737 + 0.3207197d*E (JD2440500 - 41600);
SW    Lac    [00001]; Min I = 2442697.4039 + 0.3207144d*E
SW    Lac    (JD2441600 - 43100) [09295]; Min I = 2443459.7476 +
SW    Lac    0.3207216d*E (JD2443100 - 44400) [09297]; Min I =
SW    Lac    2444856.8064 + 0.3207184d*E (JD2444400 - 44900)
SW    Lac    [00001]; since JD2444900 - see Table.
SW    Lac    Shape of the light curve, depths of minima and heights
SW    Lac    of maxima vary.
TW    Lac    d = 0.018P. P var. Min I = 2424387.332 + 3.0374936d*E
TW    Lac    (JD2424380 - 34000) [02389]; Min I = 2434049.593 +
TW    Lac    3.037520d*E (JD2434000 - 36560) [03115];
TW    Lac    since JD2441500 - see Table.
TZ    Lac    In the region of the open cluster NGC 7243.
UW    Lac    Depth of Min II 0.05m; d = 0.028P. P var.
UW    Lac    Min I = 2429158.17 + 5.2902d*E (JD2414580 - 29440)
UW    Lac    [01813]; Min I = 2429158.17 + 5.290000d*E
UW    Lac    (JD2429440 - 35800) [03115]; since JD2436800 - see Table.
UW    Lac    Apsidal motion is possible [09300].
UY    Lac    d = 0.022P.
UZ    Lac    P var?
VX    Lac    P var. Min = 2424791.488 + 1.0744891d*E
VX    Lac    (JD2424700 - 32400); Min = 2432479.477 + 1.0744991d*E
VX    Lac    (JD2432400 - 40510); Min = 2440750.971 +
VX    Lac    1.0744881d*E (JD2440750 - 43000) [07552];
VX    Lac    since JD2443000 - see Table.
VY    Lac    Min II 10.6. P var? Min I = 2434629.392 + 1.036245d*E
VY    Lac    (JD2424700 - 39830) [01804]; since JD2440080 - see Table.
WY    Lac    Light variations with P = 850d and A = 1.5m are
WY    Lac    superimposed by variations with P = 50d and A = 1m.
XX    Lac    In the region of the open cluster NGC 7243.
XZ    Lac    P var.
AG    Lac    Min II 14.0.
AR    Lac    Min II 6.43; Min II - Min I = 0.5018P; dI = 0.045P; DII =
AR    Lac    0.13P; dII = 0.00P. P var. Min I = 2426624.378 +
AR    Lac    1.983244d*E (JD2415300 - 26800) [09309]; Min I =
AR    Lac    2429535.739 + 1.9832125d*E (JD2426800 - 36000)
AR    Lac    [09312]; Min I = 2437018.414 + 1.983252d*E
AR    Lac    (JD2436000 - 37500) [00001]; since JD2437500 - see Table.
AR    Lac    There is a square term in the elements
AR    Lac    given in the Table:  - 5.24d*10**(-9)*E**2.
AR    Lac    Shape of the light curve varies; there is a
AR    Lac    distortion wave with A up to 0.13mV migrating in the
AR    Lac    direction of decreasing phases with P ~2.5 yr. Spectrum
AR    Lac    investigations [01816, 09315, 9316].
AU    Lac    Min II 12.2; Min II - Min I = 0.53P.
AW    Lac    Min II 11.2.
BH    Lac    Hydrogen lines in the spectrum are sharp and deep [03149].
BL    Lac    Z = 0.07; B-V =  +1.0. Light curve graph [06784].
BM    Lac    The elements are valid in the interval JD2425200 - 26250.
BT    Lac    There is a square term in the elements: -0.0004d*E**2.
BT    Lac    Epoch of Max brightness is given in the Table.
BT    Lac    Mean brightness varies in the range 13.8m - 15.2m with
BT    Lac    P = 654d. Mean amplitude of the shortperiodical variations
BT    Lac    is ~1.5m. There occur changes of primaries and
BT    Lac    secondaries minima into each other.
BU    Lac    The main variation is superimposed by waves with a
BU    Lac    possible period -200d.
CG    Lac    Min II 14.0.
CM    Lac    Min II 8.53; DII = 0.12P.
CN    Lac    Min II 12.6. In the region of the
CN    Lac    open cluster NGC 7209. Not member of the cluster.
CO    Lac    Min II 10.79. Apsidal motion with
CO    Lac    P = 42.3 yr is observed. There is a periodic term in
CO    Lac    The elements given in the Table: -0.0133d cos(157.7deg +
CO    Lac    0.0359deg*E). Min II = 2427534.8439 + 1.5422075d*E +
CO    Lac    0.0133d cos(157.7deg + 0.0359deg*E).
CS    Lac    Min II 9.4.
CZ    Lac    Delta(S) = 1. P var. Max = 2432878.234 + 0.43210346d*E
CZ    Lac    (JD2428700 - 39400) [01442]; Max = 2443081.309 +
CZ    Lac    0.4319850d*E (JD2439400 - 43100) [05839]; Max =
CZ    Lac    2444080.122 + 0.432114d*E (JD2443800 - 44100)
CZ    Lac    [09009]; since JD2445100 - see Table.
DD    Lac    VB A (B 9.2m, 69", 16deg).  P var. Max = 2421914.178 +
DD    Lac    0.19309018d*E - 0.001798d*10**(-8)*E**2 (JD2421400 -
DD    Lac    37600) [05711]; since JD2443000 - see Table.
DD    Lac    According to [09337] simultaneously the pulsations with
DD    Lac    the following periods are observed (the corresponding AB
DD    Lac    values are given in the brackets): P1 = 0.193082d (0.080m),
DD    Lac    P2 = 0.197382d (0.034m), P3 = 0.182115d (0.020m),
DD    Lac    P4 = 0.187438d (0.016m), P5 = 0.095109d (0.010m),
DD    Lac    P6 = 0.23583d (0.008m). A var; 0.04m <= A <= 0.12m.
DE    Lac    Delta(S) = 5. P var. Max = 2428807.130 + 0.2536940d*E
DE    Lac    (JD2427000 - 33000); Max = 2433005.766 + 0.2536929d*E
DE    Lac    (JD2433000 - 39100) [03378]; since JD2442000 - see Table.
DF    Lac    [A/H] = 0.2.
DG    Lac    P var. Min = 2426266.355 + 2.206435d*E (JD2426200 - 40000)
DG    Lac    [04961]; since JD2440000 - see Table.
DH    Lac    P var. Max = 2418240 + 284.8d*E (JD2418000 - 27350);
DH    Lac    since JD2427300 - see Table.
DM    Lac    Erroneously labeled VV306, instead of VV307, in the chart [05862].
DO    Lac    According to [00085], EA.
EG    Lac    P > 50d? [05386].
EM    Lac    Min II 13.09.
EN    Lac    VB A (B 11.32mV, 27", 345deg; C 9.0mV, 62", 48deg); SB1
EN    Lac    (Porb = 12.0968d). Eclipsing system with a pulsating
EN    Lac    primary component of BCEP type. Depth of Min I 0.05mB.
EN    Lac    Min I = 2444909.4339 + 12.096816d*E; D = 0.015P,
EN    Lac    d = 0.000P. Simultaneously pulsations are
EN    Lac    observed with the periods P1 = 0.169170d, P2 = 0.170770d,
EN    Lac    P3 = 0.181692d [09346]. The corresponding amplitudes
EN    Lac    of pulsations vary. The values of the amplitudes in
EN    Lac    B system are as follows: A1 = 0.046m, A2 = 0.024m,
EN    Lac    A3 = 0.022m (1952 - 1965); A1 = 0.016m, A2 = 0.010m,
EN    Lac    A3 = 0.014m (1977); A1 = 0.010m, A2 = 0.014m, A3 = 0.023m
EN    Lac    (1980 - 81). 0.01m <= A <= 0.11m.
EO    Lac    Min II 12.9; Min II - Min I = 0.485P.
EP    Lac    Depth of Min II 0.04m.
ER    Lac    Depth of Min II 0.05m:.
ES    Lac    Min II 11.6; Min II - Min I = 0.57P.
ES    Lac    Apsidal motion is possible:
ES    Lac    Min II = 2433582.95 + 4.459451d*E [09347].
EU    Lac    The chart in [05862] is wrong.
EV    Lac    VB A (B 12.74mB, 10", 260deg, 1949); mu alpha = -0.065s,
EV    Lac    mu delta = -0.46". Dark companion (A = 0.0206", P = 45 yr,
EV    Lac    E = 0.5) [09348]. In 1979 sinusoidal light oscillations
EV    Lac    were observed in the range 10.20m - 10.27mV:
EV    Lac    Min = 2444037.576 + 4.378d*E [09349]. In 1974 - 76 such
EV    Lac    periodicity was not observed [09350].
EW    Lac    Non-radial pulsations with P = 0.7d - 0.8d
EW    Lac    are also possible [09351, 09352].
EX    Lac    d = 0.050P.
FQ    Lac    A var; P var. Elements given in the Table are valid in the
FQ    Lac    intervale JD2427950 - 31700.
FU    Lac    d = 0.013P.
GS    Lac    Min II 15.2.
GX    Lac    Min II 10.23.
HK    Lac    SB1 (Porb = 24.4284d [09355]).
HM    Lac    Depth of Min II 0.05m.
HN    Lac    Min II 14.7.
HQ    Lac    Erroneously labeled VV307, instead of VV306, in the chart [05862].
HR    Lac    Min II 14.3.
HT    Lac    In the region of the open cluster NGC 7209.
HW    Lac    Min II 14.8.
HX    Lac    Min II 14.8.
HZ    Lac    Min II 15.0.
IM    Lac    Min II 13.2.
IN    Lac    E?
IP    Lac    Min II 14.0.
IR    Lac    Min II 15.4; d = 0.03P.
IT    Lac    P var.
IU    Lac    Min II 13.5.
IY    Lac    Blazhko effect?
IZ    Lac    Min II 12.7.
KO    Lac    Min II 14.7.
KP    Lac    P < 1d.
KR    Lac    Min II 15.8; dII = 0.05P.
KS    Lac    Depth of Min II 0.03m.
KU    Lac    Depth of Min II 0.03m.
LU    Lac    Min II 15.32.
LW    Lac    d = 0.03P. Depth of Min II 0.03m?
LY    Lac    Min II 12.6.
LZ    Lac    Min II 12.5.
MO    Lac    d = 0.04P. Depth of Min II 0.05m.
MP    Lac    Min II 12.5.
MV    Lac    Min II 15.0.
MZ    Lac    Min II 12.1; Min II - Min I = 0.713P.
MZ    Lac    Min II = 2433872.702 + 3.158719d*E. Elements for Min I
MZ    Lac    are given in the Table.
NN    Lac    d = 0.02P. np (usually brighter) component of a close pair.
NN    Lac    The range of combined brightness is given in the Table.
NO    Lac    Depth of Min II 0.03m.
NR    Lac    Min II 13.4. Sp (brighter) component of a close pair. The
NR    Lac    range of combined brightness is given in the Table.
NU    Lac    EW?
NW    Lac    Min II 13.9. Close binary, the components of which are
NW    Lac    equal in brightness at minimum light. The range of
NW    Lac    combined brightness is given in the Table.
OO    Lac    Min II 12.8.
OV    Lac    150d <= P <= 200d.
OX    Lac    Depth of Min II 0.04m.
PP    Lac    Min II 12.0.
PT    Lac    Min II 15.4.
PZ    Lac    In the region of the open cluster NGC 7243.
QQ    Lac    In the region of the open cluster NGC 7243.
QU    Lac    Depth of Min II 0.04m.
V0335 Lac    Min II 15.8.
V0338 Lac    In the region of the open cluster IC 1434.
V0339 Lac    P = 3.4084964d?
V0340 Lac    Min II 12.4; Min II - Min I = 0.762P;
V0340 Lac    Min II = 2432858.521 + 19.943102d*E.
V0340 Lac    Elements for Min I are given in the Table.
V0342 Lac    Min II 12.9.
V0343 Lac    Min II - Min I = 0.57P. Depth of Min II 0.03m:.
V0344 Lac    Min II 13.0. Min I = 2433873.5784 + 0.39222768d*E
V0344 Lac    (JD2432800 - 35800); since JD2445200 - see Table.
V0345 Lac    Min II 11.6; Min II - Min I = 0.340P; DII = 0.040P;
V0345 Lac    dII = 0.014P. Apsidal motion is possible.
V0347 Lac    VB.
V0350 Lac    VB A (B 9.7m, 66", 94deg); SB1 (P = 17.755d [09356]).
V0350 Lac    Min II 6.45 [07468]. Mean magnitude varies. See also [08933].
V0355 Lac    Northern component of a pair.
V0360 Lac    SB2 (P = 10d [09357]). Min II 5.93.
V0362 Lac    VB A (B 13.2m, 1.8", 49deg).
V0363 Lac    VB A (B 11.3m, F6 III - V:, 6.3", 325deg).
V0364 Lac    Min II 9.15; Min II - Min I = 0.52P; dI = 0.003P,
V0364 Lac    DII = 0.077P, dII = 0.009P.
V0412 Lac    SB, Porb = 41.95yr.
V0413 Lac    SB, Porb = 2.9833d.
V0442 Lac    Quasi-periodic brightness variations of a planetary nebula, possibly
V0442 Lac    due to variable mass loss or pulsations.
V0450 Lac    MinII 13.65.
V0457 Lac    A twice shorter period is not excluded.
V0468 Lac    Multiperiodic.
R     Leo    P var. Max = 2385112 + 312.43d*E (JD2385100 - 2402500);
R     Leo    Max = 2402929 + 314.33d*E (JD2402500 - 11500);
R     Leo    Max = 2411416 + 308.93d*E (JD2411500 - 16500);
R     Leo    Max = 2416984 + 317.84d*E (JD2416500 - 22500);
R     Leo    Max = 2423328 + 312.75d*E (JD2422500 - 27000);
R     Leo    Max = 2427081 + 307.40d*E (JD2427000 - 30000);
R     Leo    Max = 2437337 + 312.13d*E (JD2430000 - 37500);
R     Leo    since JD2437500 - see Table. SiO, H2O, OH maser.
S     Leo    P var. Max = 2420654 + 189.24d*E (JD2420200 - 26100);
S     Leo    Max = 2426142 + 185.92d*E (JD2426100 - 28100);
S     Leo    since JD2428100 - see Table.
V     Leo    H2O maser.
W     Leo    P var. Max = 2434651 + 385.41d*E (JD2409500 - 35000);
W     Leo    since JD2437500 - see Table. OH maser.
Y     Leo    P var. Min = 2422372.520 + 1.6860978d*E (JD2418000 - 23500)
Y     Leo    [02389]; Min = 2422372.5368 + 1.68607314d*E
Y     Leo    (JD2423500 - 38600) [09307]; since JD2438600 - see Table.
Y     Leo    There is periodic term in the elements given in the Table:
Y     Leo    +0.00375d*sin(0.21487deg*E + 141.7deg). Depth of Min II
Y     Leo    0.1m IR.
RR    Leo    Delta(S) = 7.1. P var. Max = 2430440.3385 + 0.45238172d*E +
RR    Leo    1.963d*10**(-10)*E**2 (1898 - 1977) [08299]; since
RR    Leo    JD2441400 - see Table.
RT    Leo    Min II 10.5.
RW    Leo    P var. Before JD2440800 Min = 2424993.458 +
RW    Leo    1.6825365d*E [03115]; since JD2440800 - see Table.
RX    Leo    Delta(S) = 6.8.
SS    Leo    P var. Max = 2415485.723 + 0.62633242d*E
SS    Leo    (JD2414000 - 22000) [00752]; since JD2422000 - see Table.
SS    Leo    [Fe/H] = -1.59.
ST    Leo    (k - b)2 = 0.08.
SZ    Leo    P var. Before JD2442500 Max = 2425331.400 +
SZ    Leo    0.5340833d*E [04157]; since JD2442500 - see Table.
SZ    Leo    Light curve shape var?
TU    Leo    Minor planet (8) Flora.
TV    Leo    P var. Max = 2419852.318 + 0.6728362d*E
TV    Leo    (JD2419000 - 28000) [00001]; since JD2437000 - see Table.
TV    Leo    (k - b)2 = -0.01.
TX    Leo    VB A (B 7.8m, 2", 157deg, 1971);
TX    Leo    A binary according to lunar occultation data: ro = 0.0005".
TX    Leo    The range of combined brightness is given.
TX    Leo    Min II 5.69; DII = 0.19P; Min II - Min I = 0.550P.
TY    Leo    Elements need confirmation.
UU    Leo    Min II 11.5. P var. Since JD2430000 - see Table.
UV    Leo    Min II 9.49; d = 0.014P. P var. Before JD2434000
UV    Leo    Min I = 2425574.302 + 0.60008516d*E [07554];
UV    Leo    since JD2434000 - see Table.
UX    Leo    Min II 10.4.
UX    Leo    Moments of Min by BBSAG contradict the tabulated elements.
UZ    Leo    Min II 10.12. P var, nonlinear term: +2.8d*10**(-12)*E**2.
XX    Leo    Min II 11.4. Period should be checked.
XY    Leo    Min II 9.80. P var. Min = 2435195.66306 + 0.2841091d*E
XY    Leo    (JD2434000 - 36500) [03392]; Min = 2437376.465 +
XY    Leo    0.28409592d*E (JD2436500 - 40000) [00001]; Min =
XY    Leo    2441005.5364 + 0.28410727d*E (JD2441000 - 44000)
XY    Leo    [09084]; since JD2444000 - see Table.
XY    Leo    The light curve shape var.
XZ    Leo    Min II 11.1.
AB    Leo    Epoch of Min is given.
AB    Leo    According to [01853], Max = 2428880 +
AB    Leo    103.2d*E (JD2414600 - 19000, 2428000 - 31600);
AB    Leo    During other time intervals cycles 75d - 125d.
AD    Leo    mu = 0.49", P = 265deg; pi = 0.20".
AD    Leo    X-ray and radio source. Astrometric binary?
AF    Leo    H2O maser.
AM    Leo    VB A (B 10.64m, 11", 270deg). Min II 9.83.
AP    Leo    Min II 9.88. P var. Min = 2414986.868 + 0.430350d*E
AP    Leo    (JD2414700 - 18600); since JD2418600 - see Table.
AP    Leo    Light curve shape var.
AQ    Leo    Elements for fundamental mode pulsations (P0) see Table.
AQ    Leo    For the first overtone: P1 var?;
AQ    Leo    P1 = 0.4101369d (1929 - 1969); P1 = 0.410130d (1957 -
AQ    Leo    1969); during 1973 - 1975 Max1 =
AQ    Leo    2441766.486 + 0.4101487d*E. delta(M0) = 0.23m,
AQ    Leo    delta(M1) = 0.46M.
AU    Leo    Vr = +7545 km/s. Variability is doubtful.
BB    Leo    [Fe/H] = -1.32.
BL    Leo    Min II14.4. P var. Since JD2442000 - see Table.
BV    Leo    Min II 16.1.
BW    Leo    Min II 15.4.
BX    Leo    [Fe/H] = -1.23.
BZ    Leo    Min II 15.8.
CD    Leo    Light curve shape var.
CE    Leo    Min II 12.5. P var?
CE    Leo    Min by BBSAG contradict the tabulated elements.
CN    Leo    Mu = 4.7", P = 235deg; pi = 0.41".
CN    Leo    Soft X-ray source, radio source.
CW    Leo    Dust envelope, 6"*4".
CW    Leo    Molecular radioemission: SiO, SiS, HCN, HC3N, CO, H2O,
CW    Leo    NH3, etc. Polarization in I band up to 24%.
CX    Leo    VB A (B 12.3m, 132deg); SB (Porb = 12685.4d).
CY    Leo    mu = 0.307", P = 141.3deg; pi = 0.022".
CY    Leo    Outside flares Delta(m) < = 0.036m; P = 600s, 822s, 1638s
CY    Leo    [06209]. A single strong flare with delta(M) = 0.61m in
CY    Leo    blue light of 10 Min duration was observed [06141],
CY    Leo    which is attributed by several authors to the presence of
CY    Leo    a red flaring companion.
DE    Leo    P = 1.2d - 2.0d?
DG    Leo    VB B (A 6.6m, A 8IV, SB2, Porb = 4.15d; B 6.9m, 0.271",
DG    Leo    211.2deg, 1980, Porb ~200yr).
DG    Leo    The range of the bombined brightness is given.
DH    Leo    SB1, Porb = 1.070354d.
DK    Leo    mu alpha = -0.097", mu delta = -0.214".
FL    Leo    Variability range according to E.M. Halbedel, IBVS No. 3502, 1990.
FX    Leo    Not a nearby star (despite having a Gl number).
GU    Leo    MinII 12.19.
GV    Leo    MinII 11.87.
HI    Leo    The depth of MinII is 0.5.
HK    Leo    Epoch of Min is given.
HM    Leo    Porb = 0.1868d.
HQ    Leo    The tabulated amplitude was probably influenced by a companion in 35" np.
HY    Leo    Porb = 0.1736d; Pspin = 0.04804d.
IK    Leo    Superhumps P = 0.056281d.
IQ    Leo    Min II = 15.2.
IU    Leo    Porb = 0.3763d.
KO    Leo    P = 0.293919d is also possible.
KT    Leo    P = 0.256494 is also possible.
KV    Leo    Multiperiodic. SB?
R     LMi    SiO, H2O, OH mazer.
T     LMi    Min II 10.97. P var. Min I = 2420573.698 + 3.019889d*E
T     LMi    (JD2420200 - 25000); Min I = 2423856.323 +
T     LMi    3.0199336d*E (JD2423800 - 35500); since JD2438400 - see
T     LMi    Table.
U     LMi    1m <= A <= 3.3m. Periodicity sometimes breaks down.
V     LMi    Delta(S) = 5.7.
Y     LMi    P var. Max = 2428636.322 + 0.52443938d*E + 0.0597d*
Y     LMi    *sin(0.0657deg*E + 27.2deg) (JD2425250 - 28500); Max =
Y     LMi    2428636.348 + 0.5244564d*E (JD2428500 - 30000)
Y     LMi    [01856]; mean elements
Y     LMi    for interval JD2432200 - 38900 are given in the
Y     LMi    Table; in this interval the period changed with the
Y     LMi    cycle of ~2100d. Blazhko effect with the period 33.4d
Y     LMi    [01856]; 07m <= A <= 1.9m, 0.19P <= m - M <= 0.44P.
RT    LMi    Min II 11.7.
RU    LMi    Spectrum description [09326].
RW    LMi    VB A (B 15.5m B, 9", 10deg). 0.3m - 2.6m K, 7.64m - 10.71m,
RW    LMi    9.7m - 14.6m R, 14.1m - 18.1m B, 14.8m - 18.6m U.
RW    LMi    Mean brightness varies. Gaseous-dust circumstellar
RW    LMi    envelope. CO emission. Spectrum description [09327].
RY    LMi    VB A (B 16.1m, dM2, 15", 126deg); mu = 0.14", P = 264deg.
RY    LMi    P0 = 215.197388s, dP0/dt = 5.6s*10**(-14)/s, A0 = 0.0440m;
RY    LMi    P1 = 304.4s, A1 = 0.0150m; P2 = 271.0s, A2 = 0.0134m;
RY    LMi    P3 = 107.6s, A3 = 0.0032m; P4 = 126.2s, A4 = 0.0028m;
RY    LMi    P5 = 119.8s, A5 = 0.0026m.
RY    LMi    Mean brightness varies by 0.05m.
WZ    LMi    MinII 12.68.
XX    LMi    MinII 12.56.
XY    LMi    MinII 11.13.
XZ    LMi    SB1?
YY    LMi    SB1?
YZ    LMi    Min II = 19.3.
AC    LMi    Porb = 0.07938d.
AD    LMi    SB1, Porb = 15.465d.
AE    LMi    Min II = 13.1.
AF    LMi    Min II = 14.5.
AG    LMi    Min II = 10.75:. A twice longer period, with equally deep minima, is also possible.
R     Lep    P var. Max = 2398883 + 436.44d*E (JD2398000 - 2412000);
R     Lep    Max = 2412849 + 418.04d*E (JD2412000 - 23000);
R     Lep    Max = 2423300 + 441.38d*E (JD2423000 - 36000);
R     Lep    since JD2436000 - see Table.
R     Lep    A var; 5.5m <= Max <= 9.5m (Possible period is more
R     Lep    than 40 years [03402]).
S     Lep    Mean magnitude varies with the cycle of 890d. H2O maser.
T     Lep    SiO maser.
U     Lep    P var. Max = 2425084.431 + 0.58147098d*E
U     Lep    (JD2411000 - 25090); Max = 2425084.431 + 0.58147377d*E
U     Lep    (JD2425080 - 37700) [03403]; since JD2436600 - see Table.
U     Lep    Delta(S) = 8.5; (k - b)2 = 0.00.
V     Lep    Min II 9.9.
Z     Lep    Min II 12.0:.
RR    Lep    Min II 10.4.
RS    Lep    Min II 9.96.
RU    Lep    P var?
RZ    Lep    S 4/4.
SS    Lep    SB2 (Porb = 258.2d [09363]).
SY    Lep    VB A (B 15.2m: V, 18", 270deg).
AM    Lep    VB B (A = HR 1696, 4.45m, B8V; B 12", 337deg, 1998).
BC    Lep    Min II = 10.70.
BH    Lep    A brown dwarf with periodic brightness variations.
S     Lib    P var. Max = 2405692 + 192.14d*E (JD2402700 - 24000);
S     Lib    Max = 2424141 + 194.74d*E (JD2424000 - 30500);
S     Lib    Max = 2431900 + 190.34d*E (JD2430500 - 37200);
S     Lib    Max = 2439203 + 197.61d*E (JD2437200 - 39300);
S     Lib    since JD2441000 - see Table. Mean value of the period is
S     Lib    given in the Table. A var (1.8m <= A <= 5m).
W     Lib    P var. Max = 2412272 + 203.76d*E (JD2412000 - 28500);
W     Lib    Max = 2428573 + 201.48d*E (JD2428500 - 34000);
W     Lib    since JD2434000 - see Table.
X     Lib    P var. Max = 2423500 + 165.75d*E (JD2413000 - 25000);
X     Lib    since JD2425000 - see Table.
Y     Lib    P var. Max = 2413452 + 275.7d*E (JD2413400 - 22000);
Y     Lib    Max = 2422273 + 272.5d*E (JD2422000 - 28000) [00458];
Y     Lib    Max = 2434921 + 277.04d*E (JD2428000 - 35000);
Y     Lib    since JD2435000 - see Table.
Z     Lib    P var. Max = 2417736 + 294.5d*E (JD2407100 - 17800);
Z     Lib    since JD2424400 - see Table.
RR    Lib    P var. Max = 2409699 + 277.4d*E (JD2409600 - 15600);
RR    Lib    Max = 2416345 + 273.2d*E (JD2416300 - 19700);
RR    Lib    Max = 2421027 + 278.6d*E (JD2421000 - 27150) [00458];
RR    Lib    since JD2427150 - see Table.
RS    Lib    P var. Max = 2413396 + 217.2d*E (JD2413300 - 20000);
RS    Lib    Max = 2420110 + 219.6d*E (JD2420000 - 27500) [00458];
RS    Lib    Max = 2429078 + 215.6d*E (JD2427500 - 35000);
RS    Lib    Max = 2438196 + 219.9d*E (JD2435000 - 42600);
RS    Lib    since JD2441700 - see Table.
RT    Lib    P var. Max = 2413776 + 254.21d*E (JD2413000 - 19000);
RT    Lib    since JD2419000 - see Table.
RU    Lib    P var. Max = 2413363 + 312.0d*E (JD2413300 - 16200);
RU    Lib    Max = 2416807 + 322.5d*E (JD2416800 - 21000);
RU    Lib    Max = 2421309 + 317.0d*E (JD2421300 - 24200);
RU    Lib    Max = 2424804 + 311.5d*E (JD2424800 - 29800) [00458];
RU    Lib    Max = 2434909 + 319.9d*E (JD2429800 - 35000); since
RU    Lib    JD2437700 - see Table.
RV    Lib    Min II 9.44.
RX    Lib    [A/H] =  -0.5. P var. Max = 2430913.6 + 24.950d*E
RX    Lib    (JD2425000 - 36300) [00266]; since JD2436300 - see Table.
SS    Lib    Min II 10.8; d = 0.030P.
ST    Lib    VB A (B 14m, 14", 0deg).
TV    Lib    Delta(S) = 2.5.
TY    Lib    d = 0.019P.
UW    Lib    [Fe/H] =  - 0.25.
VV    Lib    P var. Max = 2424268.474 + 0.4781418d*E
VV    Lib    (JD2419800 - 2425000); since JD2425000 - see Table.
VW    Lib    Observations given in
VW    Lib    [00293] contradict the elements given in the Table.
VY    Lib    P var? [03506].Delta(S) = 6.
VZ    Lib    Min II 10.55; dI = 0.000P; dII = 0.005P. P var. Min I =
VZ    Lib    2429022.227 + 0.358053d*E (JD2428600 - 30400)
VZ    Lib    [09368]; Min I = 2430899.223 + 0.358448d*E
VZ    Lib    (JD2430400 - 32400) [02532]; since JD2444330 - see Table.
YZ    Lib    Min II 12.9.
AA    Lib    P var? The elements are valid in the interval
AA    Lib    JD2427800 - 29600.
AF    Lib    The chart in [06286] has south on top.
AP    Lib    Z = 0.0486.
AQ    Lib    [Fe/H] = -0.60.
BE    Lib    The chart in [06286] is wrong.
BH    Lib    Recommended chart in [06286]: part III, page 50.
BT    Lib    Min II 12.3.
BW    Lib    The chart in [06286] is wrong.
CG    Lib    [Fe/H] = -1.82. P var. Max = 2438592.287 + 0.3068674d*E
CG    Lib    (JD2427800 - 39600) [07557]; since JD2439600 - see Table.
CQ    Lib    The coordinates in [01870] are wrong.
CZ    Lib    The chart in [06286], part I, page 40 is wrong. Recomended
CZ    Lib    chart in [06286]: part III, page 52.
EH    Lib    Delta(S) = 0. 9.35m <= Max < = 9.49m V;
EH    Lib    Max (A) = 2442162.556 + 0.273778d*E [09336].
ES    Lib    Min II 7.33.
EU    Lib    70d <= P <= 90d.
FI    Lib    90d <= P <= 110d.
FS    Lib    OH emission.
FX    Lib    Spectrum description  [06167, 09371].
KZ    Lib    MinII 11.22.
LZ    Lib    Deviations from the light curve with the tabulated period reveal P2 = 0.334339d, also with an EW light curve. A quadruple system?
MR    Lib    Blazhko effect, P = 41.7d.
NY    Lib    P = 0.361945d is also possible.
OO    Lib    P = 0.462571d is also possible.
OR    Lib    The mean brightness varies slowly.
OZ    Lib    Superposed variations with an amplitude up to 0.5m and a period about 53d.
PT    Lib    Min II = 14.6. A twice shorter period and type RRC are possible.
PW    Lib    P varies? [001].
QZ    Lib    Superhumps, P= 0.064602d.
V0339 Lib    Min II = 14.2.
V0351 Lib    Min II = 14.0.
del   Lib    VB A (B 11.3m, 9", 351deg; C 12.80m, 67", 90deg); Min II
del   Lib    4.98. P var?
S     Lup    VB A (B = X Lup, 13", 176deg). P var. Max = 2411950 +
S     Lup    347.81d*E (JD2411950 - 14000); Max = 2414040 +
S     Lup    339.31d*E (JD2414000 - 19000); Max = 2419135 +
S     Lup    345.12d*E (JD2419000 - 26000); Max = 2426038 +
S     Lup    336.60d*E (JD2426000 - 29500); Max = 2429743 +
S     Lup    345.15d*E (JD2429500 - 35000); since JD2437600 - see Table.
X     Lup    VB B (A = S Lup).
Y     Lup    P var. Max = 2424691 + 408.15d*E (JD2423000 -
Y     Lup    25500); Max = 2425503 + 394.81d*E (JD2425500 -
Y     Lup    30250); Max = 2430641 + 407.75d*E (JD2430250 -
Y     Lup    35000); since JD2437900 - see Table.
RU    Lup    Sometimes varies quasiperiodically: P1 = 3.5457d, P2 =
RU    Lup    3.8375 [02412]. H2O maser.
RY    Lup    Quasiperiodicity: P = 3.7609d [09366].
SX    Lup    Min II 11.8.
TY    Lup    The chart in [06286] is wrong.
UX    Lup    [A/H] = -0.9. P var. P = 16.2403d (JD2411526 -
UX    Lup    14040); P = 16.2065d (JD2414040 - 24016); P =
UX    Lup    16.2492d (JD2424016 - 25638); P = 16.1794d
UX    Lup    (JD2425638 - 26449); P = 16.2241d (JD2426449 - 29693)
UX    Lup    [05387].
VV    Lup    Close northern companion.
VZ    Lup    P var? Light curve shape var?
CC    Lup    The chart in [06286] is wrong.
CW    Lup    The charts in [06286] are wrong.
CX    Lup    Min II 12.8.
CY    Lup    High Max every 360d, especially faint Min 80d before
CY    Lup    these high Max.
DG    Lup    Min II 15.1.
DQ    Lup    The chart in [06286] is wrong.
DY    Lup    In [00087] the information on variability of DY Lup is
DY    Lup    accompanied by the coordinates of DZ Lup and vice versa.
DY    Lup    The chart for DY Lup in [06286] is labeled DZ Lup, the
DY    Lup    chart for DZ Lup in [06286] is wrong.
DZ    Lup    In [00087] the information on variability of DY Lup is
DZ    Lup    accompanied by the coordinates of DZ Lup and vice versa.
DZ    Lup    The chart for DY Lup in [06286] is labeled DZ Lup, the
DZ    Lup    chart for DZ Lup in [06286] is wrong.
EL    Lup    VB.
ER    Lup    P2 = 140d.
EU    Lup    The chart in [06286] is wrong.
FK    Lup    Min II 10.7:.
FM    Lup    The chart in [02385] is wrong.
FR    Lup    Deep Min II.
FT    Lup    Min II 9.98. dI = 0.025P?, dII >= 0.066P. P var.
FT    Lup    Before JD2439300 Min I = 2427987.310 + 0.470089d*E
FT    Lup    [03948]; since JD2445000 - see Table. All the observations
FT    Lup    are well represented also by the elements:
FT    Lup    Min I = 2445061.834 + 0.470083d*E - 0.114d*10**(-9)*E**2
FT    Lup    [09360]. Light curve shape var?
FV    Lup    Min II 11.2.
GG    Lup    Min II 5.8.
GN    Lup    VB A (B 10.2m vis, 10", 98deg).
GO    Lup    Relatively short P.
GW    Lup    In the dark nebula Barnard 228.
HL    Lup    The initial identification with 2U 1543 - 47 is wrong.
HL    Lup    2U 1543 - 47 = IL Lup.
HM    Lup    B - V: +1.12.
HN    Lup    B - V: +1.55, +1.68.
HO    Lup    B - V: +0.70, +0.81.
OO    Lup    A twice shorter period is not excluded.
OR    Lup    SB3, G1IV/V + G8:V/IV: + K0:V.
OT    Lup    A twice shorter period is not excluded.
OU    Lup    MinII - MinI = 0.28P.
PP    Lup    MinII - MinI = 0.28P.
PQ    Lup    Blazhko effect, P=48.8d.
PS    Lup    P varies, current elements are given.
PZ    Lup    Min II = 10.67.
QQ    Lup    Min II = 13.2.
QT    Lup    Min II = 12.80.
QU    Lup    Min II = 10.53. dP/dt = -0.61 x 10^{-5} d/yr. VB AB (11.3, 11.3, 0.8", 326deg, 1991).
QV    Lup    Min II = 11.68.
QZ    Lup    Min II = 8.43:.
V0339 Lup    Blazhko effect, P = 49.5d.
V0353 Lup    Min II = 12.7.
V0363 Lup    Min II = 11.85.
V0372 Lup    OH, SiO maser.
V0378 Lup    Min II = 11.0.
V0379 Lup    Min II = 9.89.
V0386 Lup    Min II = 11.3.
alf   Lup    VB A (B 14.0m, 27.6", 232deg, 1901).
alf   Lup    Soft X-ray source. P2 = 3.145d is possible [08417].
gam   Lup    SB, Porb = 2.8081d.
del   Lup    Less probable variant of elements:
del   Lup    Max = 2441045.160 + 0.14273*E.
R     Lyn    S 4/5E - S 6/6 - .
S     Lyn    VB A (B 14m, 12.6", 155deg). P var. Max = 2414564 +
S     Lyn    300.26d*E (JD2414500 - 27400); Max = 2434241 +
S     Lyn    294.42d*E (JD2427400 - 35100); Max = 2440225 +
S     Lyn    300.44d*E (JD2435100 - 40220); since
S     Lyn    JD2440220 - see Table.
T     Lyn    P var. Max = 2425012 + 419.0d*E (JD2412800 - 34700);
T     Lyn    since JD2434700 - see Table.
U     Lyn    H2O, OH emission. P var. Max = 2417168 +
U     Lyn    440.3d*E (JD2417100 - 26000) [00458]; Max =
U     Lyn    2435908 + 432.05d*E (JD2426000 - 36000); Max =
U     Lyn    2439898 + 447.1d*E (JD2436000 - 40000); since
U     Lyn    JD2440000 - see Table.
V     Lyn    Cycles 55d and 87d replace one another. Mean brightness
V     Lyn    varies.
Y     Lyn    SB.
RR    Lyn    VB A (B 10m, 50"). Min II 5.90; Min II = 2438051.3115 +
RR    Lyn    9.945074d*E; E = 0.081; Min II - Min I = 0.45P (JD2437700).
RW    Lyn    [Fe/H] = -1.37.
RZ    Lyn    Min II 10.8.
SW    Lyn    Min II 9.65; dI = 0.038P. P var. Min I = 2425643.323 +
SW    Lyn    0.6440661d*E (JD2425640 - 35850) [02742]; Min I =
SW    Lyn    2438795.8016 + 0.6440520d*E (JD2438380 - 840)
SW    Lyn    [09387]; Min I = 2440614.0107 + 0.6440729d*E
SW    Lyn    (JD2439500 - 40620) [00001]; Min I = 2442786.4493 +
SW    Lyn    0.6440677d*E (JD2440650 - 42790) [07292];
SW    Lyn    since JD2442780 - see Table.
SX    Lyn    Min II 10.1. P var. Min I = 2428636.375 + 2.0225615d*E
SX    Lyn    (JD2427400 - 34700) [00519]; Min I = 2442561.424 +
SX    Lyn    2.0225172d*E (JD2442400 - 44000); since JD2444000 - see
SX    Lyn    Table.
SZ    Lyn    SB (Porb = 1146d, E = 0.26 [09388]). Delta(S) = 0.
SZ    Lyn    There is a periodical term in the elements:
SZ    Lyn    -0.00573d cos 2pi (EP0/P1 + 0.007); P0 = 0.120534920d,
SZ    Lyn    P1 = 1150d. Amplitude and shape of the light curve vary.
TT    Lyn    Delta(S) = 7.
TV    Lyn    [Fe/H] = -0.99.
TW    Lyn    Delta(S) = 10. P var. Max = 2418676.804 + 0.4817201d*E
TW    Lyn    (JD2418670 - 20155); Max = 2420155.685 + 0.4816929d*E
TW    Lyn    (JD2420155 - 27480); Max = 2427479.359 + 0.4817481d*E
TW    Lyn    (JD2427480 - 28630);
TW    Lyn    Max = 2428627.310 + 0.4818529d*E (JD2428620 - 37800)
TW    Lyn    [02819]. Since JD2445000 - see Table.
TZ    Lyn    Epoch of Min brightness is given.
UU    Lyn    Min II 11.82.
UV    Lyn    Min II 9.78.
UZ    Lyn    VR var (P = 0.065d [09392]).
VV    Lyn    VB A (B 11.76m, 38.6",354deg); SB; mu alpha = -0.0285S,
VV    Lyn    mu delta = -0.274".
VW    Lyn    P1 = 590s, P2 = 260s [09393].
CW    Lyn    Type RRC: is also possible.
DY    Lyn    MinII 10.16.
EO    Lyn    Min II = 14.1.
EQ    Lyn    Porb = 0.0599d.
EZ    Lyn    Brightenings and mini-outbursts between superoutburts, 16.5m - 17.1mV, with oscillations (Delta V about 0.2m, P = 0.0295d). Superhumps in superoutbursts: P = 0.0597d.
FG    Lyn    Min II = 11.00.
FH    Lyn    Porb = 0.2890d.
FI    Lyn    Min II = 10.18.
FL    Lyn    Possible Porb = 0.0687d. Superhumps P = 0.06921d.
FN    Lyn    Min II = 10.36.
FT    Lyn    Min II = 13.08.
S     Lyr    P var. Max = 2416186 + 432.01d*E (JD2415700 - 20100);
S     Lyr    Max = 2420961 + 445.83d*E (JD2420900 - 26500);
S     Lyr    Max = 2426748 + 429.01d*E (JD2426500 - 30700);
S     Lyr    Max = 2432357 + 441.88d*E (JD2432000 - 34600);
S     Lyr    since JD2442500 - see Table.
U     Lyr    VB A (B 13.0m, 9.4", 182deg). P var. Max = 2418345 +
U     Lyr    459.22d*E (JD2418000 - 27000); since JD2432000 - see
U     Lyr    Table.
V     Lyr    OH maser.
W     Lyr    P var. Max = 2415578 + 198.39d*E (JD2413000 - 19000);
W     Lyr    Max = 2420322 + 194.99d*E (JD2419000 - 25500);
W     Lyr    Max = 2431326 + 198.97d*E (JD2427000 - 31500);
W     Lyr    Max = 2432494 + 195.11d*E (JD2431500 - 36500);
W     Lyr    since JD2437500 - see Table.
Y     Lyr    Delta(S) = 0.8.
Z     Lyr    P var. Max = 2418150 + 285.07d*E (JD2417500 - 22200);
Z     Lyr    Max = 2423600 + 291.37d*E (JD2422200 - 29500);
Z     Lyr    Max = 2430000 + 284.00d*E (JD2429500 - 36800);
Z     Lyr    since JD2436800 - see Table.
RR    Lyr    mu alpha = -0.11", mu delta = -0.19". [Fe/H] = -1.14;
RR    Lyr    Delta(S) = 6. Blazhko effect of variable
RR    Lyr    amplitude (practically to complete disappearance of
RR    Lyr    Blazhko effect); Pi = 40.8d. Variations of Max light
RR    Lyr    phase up to 0.14P; magnitude in Max var in the range
RR    Lyr    up to 0.6m, that in Min var in the range up to 0.1m
RR    Lyr    [03418].According to [07270], a cycle ~4 yr is present
RR    Lyr    in Blazhko effect amplitude changes; at the end of
RR    Lyr    the cycle the Blazhko effect phase changes abruptly
RR    Lyr    by 0.25Pi. Magnetic field strength varies with the
RR    Lyr    pulsational period [09339].
RR    Lyr    P var. Max = 2414856.480 + 0.56682069d*E
RR    Lyr    (JD2414800 - 18800); Max = 2421854.052 + 0.56685169d*E
RR    Lyr    (JD2418800 - 26500) [09379]; Max = 2426571.3828 +
RR    Lyr    0.56684333d*E (JD2426500 - 32500) [09338]; Max =
RR    Lyr    2438215.9492 + 0.566830d*E (JD2438000 - 41000)
RR    Lyr    [05238]; Max = 2438215.9492 + 0.56683313d*E
RR    Lyr    (JD2441000 - 42900) [09338]; since JD2442900 - see Table.
RS    Lyr    P var. Max = 2415566 + 299.38d*E (JD2415000 - 24000);
RS    Lyr    Max = 2425176 + 308.08d*E (JD2424000 - 37200);
RS    Lyr    since JD2437200 - see Table.
RT    Lyr    P var. Max = 2437022 + 250.85d*E (JD2415000 - 39000);
RT    Lyr    since JD2439000 - see Table.
RU    Lyr    P var. Max = 2415983 + 370.70d*E (JD2415900 - 33000);
RU    Lyr    Max = 2433035 + 363.0d*E (JD2433000 - 41000);
RU    Lyr    since JD2441000 - see Table.
RV    Lyr    D = 0.015P. P var. Min = 2415949.7096 + 3.599007d*E
RV    Lyr    (JD2412185 - 16000); Min = 2415949.7096 +
RV    Lyr    3.599046d*E (JD2416000 - 21400) [00001];
RV    Lyr    Min = 2432015.671 + 3.5989845d*E (JD2421400 - 32000);
RV    Lyr    Min = 2432015.671 + 3.5990235d*E (JD2432000 -
RV    Lyr    39300) [09085]; since JD2442000 - see Table.
RW    Lyr    OH, H2O maser.
RX    Lyr    P var. Max = 2416226 + 249.94d*E (JD2415000 - 28800);
RX    Lyr    since JD2428800 - see Table.
RZ    Lyr    P var. Max = 2416415.360 + 0.51127069d*E
RZ    Lyr    (JD2413000 - 19000) [00001]; Max = 2426161.4375 +
RZ    Lyr    0.51124948D*E (JD2426000 - 38000) [00323];
RZ    Lyr    since JD2438000 - see Table.
RZ    Lyr    Blazhko effect, height of Max varies: 10.6m - 10.9m,
RZ    Lyr    Max (Delta(m)) = 2430904.3 + 116.654d*N + 0.01034d*N**2;
RZ    Lyr    Min (Delta(m)) - Max (Delta(m)) = 59.3d [03419].
RZ    Lyr    [Fe/H] = -1.69; Delta(S) = 10.0.
SS    Lyr    P var. Max = 2421695 + 350.48d*E (JD2416000 - 22500);
SS    Lyr    Max = 2429991 + 355.22d*E (JD2429000 - 38000); since
SS    Lyr    JD2438000 - see Table.
SZ    Lyr    According to [05750], during JD2434665 - 35044 the
SZ    Lyr    amplitude was twice smaller than usual (due to the depth
SZ    Lyr    of Min), and a temporary phase shift by 0.5P occured.
TT    Lyr    d = 0.010P; Min II 9.44.
TW    Lyr    VB A (B 15.2m pg, 14".70deg, 1912).
TY    Lyr    P var. Max = 2419285 + 336.49d:*E (JD2419000 - 23700);
TY    Lyr    Max = 2423985 + 329.79d*E (JD2423700 - 31250);
TY    Lyr    since JD2438600 - see Table.
TZ    Lyr    VB A (B 12.29m, 2.54", 2.5deg). Min II 11.05. P var.
TZ    Lyr    Min I = 2420669.480 + 0.5288234d*E (JD2420000 - 38000);
TZ    Lyr    since JD2438000 - see Table.
UX    Lyr    B - V: +0.11, +0.47.
UZ    Lyr    d = 0.012P:. P var. Min = 2424268.474 + 1.891253d*E
UZ    Lyr    (JD2422500 - 25500) [02087]; since JD2425500 - see Table.
AA    Lyr    Min II 13.5.
AH    Lyr    d = 0.03P. Min II 12.1.
AK    Lyr    Min II 12.9.
AL    Lyr    P var. Max = 2427865.82 + 12.9837d*E (JD2414800 - 28000)
AL    Lyr    [00001]; Max = 2432889.03 + 12.98047d*E
AL    Lyr    (JD2428000 - 35500) [04427]; since JD2435500 - see Table.
AQ    Lyr    P var. Max = 2425301.592 + 0.3571721d*E
AQ    Lyr    (JD2425300 - 29000); Max = 2428944.739 + 0.3571285d*E
AQ    Lyr    (JD2429000 - 30200); Max = 2430158.976 + 0.3571611d*E
AQ    Lyr    (JD2430200 - 33900); Max = 2433909.178 + 0.3571861d*E
AQ    Lyr    (JD2433900 - 35700); during JD2435700 - 37800 - see Table.
AQ    Lyr    Blazhko effect? According to visual observations,
AQ    Lyr    0.4m <= Delta(m) <= 1.2m.
AY    Lyr    Cycles of supermaxima 188.9d - 212.8d.
AY    Lyr    Superhumps period: Ps = 0.07552d [06249].
BF    Lyr    P var. Max = 2425296 + 130d*E (JD2425300 - 800);
BF    Lyr    During JD2429045 - 570 - see Table.
BH    Lyr    P var. Max = 2413712.358 + 0.6129028d*E
BH    Lyr    (JD2413712 - 27927); Max = 2434472.547 + 0.6128941d*E
BH    Lyr    (JD2434472 - 36102); since JD2436423 - see Table.
BQ    Lyr    Delta(S) = 0:.
BV    Lyr    d = 0.025P.
CC    Lyr    P var. Max = 2433182.7 + 24.028d*E (JD2426100 - 33400);
CC    Lyr    Max = 2437078.8 + 24.200d*E (JD2433400 - 37100) [00001];
CC    Lyr    Max = 2439418.5 + 24.185d*E (JD2437100 - 39420) [05644];
CC    Lyr    since JD2440400 - see Table. Light curve shape var?
CC    Lyr    [A/H] = -2.2.
CV    Lyr    Possible superposition of P2 = 135d.
CX    Lyr    P var. Max = 2418596.111 + 0.616689d*E
CX    Lyr    (JD2414880 - 20000); Max = 2427696.396 + 0.616669d*E
CX    Lyr    (JD2427530 - 30610); since JD2433000 - see Table.
CX    Lyr    Delta(S) = 7:.
DD    Lyr    P var. Max = 2425494.334 + 0.372610d*E (JD2418900 - 27600)
DD    Lyr    [00001]; since JD2427600 - see Table.
DF    Lyr    Min II 13.4.
DI    Lyr    P var. Max = 2437160.310 + 0.4174486d*E (JD2437160 - 39293);
DI    Lyr    Max = 2439293.468 + 0.4178451d*E (JD2439293 - 40768);
DI    Lyr    since JD2440768 - see Table.
DN    Lyr    P2 = 600d.
DR    Lyr    [Fe/H] =  -1.41; Delta(S) =7.4.
DU    Lyr    Min II 13.3.
EN    Lyr    B - V: + 0.40. + 0.43. P var. Delta(m) var.
EP    Lyr    Max I Phase = 0.20P; Min II 10.36m - 10.58m,  Phase = 0.50P;
EP    Lyr    Max II 10.01m - 10.10m,  Phase = 0.70P.
EP    Lyr    Secondary oscillations: P2 = 45.1d,  P3 = 7067d [09354].
EW    Lyr    P var; nonlinear term:
EW    Lyr    +0.00210d*10**(-6)*E**2 (JD2426500 - 45500);
EW    Lyr    since JD2442000 the observations are represented also by
EW    Lyr    the elements: Min = 2445597.391 + 1.948763d*E [07037, 00001].
EX    Lyr    [Fe/H] = -0.63; Delta(S) = 2.5.
EZ    Lyr    VB A (B 12.3m, 14", 302deg, 1934). P var. Since
EZ    Lyr    JD2426577 - see Table. Delta(S) = 7.1.
FG    Lyr    VB A (B 14m, <10"). d = 0.035P. P var?
FH    Lyr    P var?
FK    Lyr    The identification with HDE 337663(G5) [00021] is wrong.
FL    Lyr    Min II 9.52,  DII = 0.05P.
FN    Lyr    B - V: +0.15, +0.48.
FO    Lyr    Min II 13.7.
GY    Lyr    The elements describe the brightest maxima. Between them
GY    Lyr    there are 2 - 3 waves of smaller amplitude. Red.
HP    Lyr    Min II 11.0.
HQ    Lyr    P var, periodic term: +30d*sin(8deg*E).
HT    Lyr    Min II 13.3.
HY    Lyr    Min II 14.1.
IK    Lyr    Blazhko effect?
IL    Lyr    According to [00569], Max = 2429375.519 + 0.377620d*E,
IL    Lyr    M - m = 0.14P:.
IO    Lyr    Delta(S) = 3.
IP    Lyr    Min II 13.3.
IW    Lyr    Min II 13.3.
IY    Lyr    Min II 14.1.
KM    Lyr    Blazhko effect: Pi = 30d, 0.14P <= M - m <= 0.20P.
KP    Lyr    ADS 11423 C (A 8.5m, B 9.7m; AB - C 77", 208deg; D 13.1m,
KP    Lyr    C - D 14", 61deg, 1904). P2 = 1300d is possible.
KR    Lyr    P var. The light curve shape var.
KT    Lyr    Min II 14.9.
KX    Lyr    Delta(S) = 0.
LQ    Lyr    [Fe/H] =  -1.39; Delta(S) = 7.2.
LR    Lyr    P var? [Fe/H] = -1.41; Delta(S) = 7.4.
LT    Lyr    Rapid variation (0.5m in an hour) were observed.
LX    Lyr    Delta(S) = 8:.
LZ    Lyr    P var. Min = 2425347.565 + 1.611143d*E (JD2425347 - 32119)
LZ    Lyr    [00569]; since JD2442870 - see Table.
MN    Lyr    Min II 14.1.
MR    Lyr    Alternative P = 0.66d:.
MS    Lyr    P < 0.5d?
MT    Lyr    Min II 16.2.
MV    Lyr    SB (Porb = 0.1336d [09373]).
MV    Lyr    Quasiperiodic fadings of different amplitude:
MV    Lyr    Min = 2425558 + 455.5d*E (JD2425500 - 30100);
MV    Lyr    Min = 2430113 + 325.3d*E (JD2430100 - 36900);
MV    Lyr    Min = 2436944 + 357.8d*E (JD2436900 - 44100) [09372].
MV    Lyr    After JD2444100 the mean brightness
MV    Lyr    level became fainter by 5m; outbursts with an amplitude
MV    Lyr    up to 3m of 1 - 2 months duration are observed [09404].
MV    Lyr    During the bright level of light, flickering up
MV    Lyr    to 0.4m in 5 Min in U bAnd is observed [00365]. Soft
MV    Lyr    X-ray source.
MV    Lyr    B - V: 0.00 +- 0.40; U - B:  -0.86 +  -1.30.
MW    Lyr    P var. Max = 2429521.386 + 0.3978817d*E (JD2427700 - 36000);
MW    Lyr    since JD2436000 - see Table.
MW    Lyr    Blazhko effect: Pi = 33.3d; the amplitude varies by 0.6m.
MZ    Lyr    Min II 14.0.
NV    Lyr    d = 0.02P:.
NW    Lyr    P var. Max = 2436483.323 + 1.6012330d*E (JD2414500 -
NW    Lyr    36400) [03506]; since JD2436400 - see Table.
NW    Lyr    B - V: +0.38, +0.86.
NY    Lyr    Min II 13.1.
NZ    Lyr    O - C vary harmonically with an amplitude +- 0.01d,
NZ    Lyr    Pi ~2500P.
OQ    Lyr    VB (B 12.1m vis, 5.3", 175deg, 1930).
OS    Lyr    40d <= P <= 60d. P2 = 400d - 500d is superimposed.
PQ    Lyr    d = 0.014P; Min II 14.9.
PS    Lyr    d = 0.02P:; Min II 11.4.
PU    Lyr    Close companions sf, s.
PV    Lyr    d = 0.03P:.
PY    Lyr    Min II 13.4. P var. Min I = 2434980.4372 + 0.38576671d*E
PY    Lyr    (JD2432700 - 36900) [04248]; since JD2442500 - see Table.
QQ    Lyr    Min II 14.6.
QT    Lyr    Min II 14.6.
QU    Lyr    Min II 13.1.
V0335 Lyr    Large scatter in the light curve.
V0336 Lyr    P var. Min = 2429965.283 + 1.9049105d*E (JD2429370 - 31590);
V0336 Lyr    during JD2438930 - 40010 - see Table.
V0337 Lyr    Large scatter in the light curve.
V0348 Lyr    Min II 16.8.
V0348 Lyr    The elements are valid during JD2444023 - 45232.
V0350 Lyr    P var. The elements are valid during JD2438280 - 45232.
V0355 Lyr    The elements are valid during JD2429322 - 45232.
V0356 Lyr    VB A (B 17.5m, 10", 120deg, [00001]).
V0361 Lyr    Min II 15.3, Max II 14.7, Max II - Min I = 0.70P.
V0361 Lyr    The elements are valid during JD2433776 - 45232).
V0374 Lyr    Faint companions np, sf.
V0380 Lyr    Faint close companion nf.
V0385 Lyr    Faint close companion sf.
V0388 Lyr    No brightenings were observed during JD2438322 - 39289.
V0389 Lyr    The elements are valid during JD2438322 - 40007.
V0390 Lyr    The elements are valid during JD2439913 - 40007.
V0401 Lyr    Min II 14.4:. The period may be spurious.
V0403 Lyr    P var?, Pi = 500 P?
V0404 Lyr    Min II 12.4.
V0406 Lyr    Min II 13.0.
V0409 Lyr    P var? The elements are valid during JD2434500 - 40000.
V0409 Lyr    Blazhko effect?
V0411 Lyr    Min II 14.4. Alternatively RRC (P = 0.291315d).
V0412 Lyr    Min II 14.1; Min II - Min I = 0.48P.
V0413 Lyr    Min II 14.8?
V0415 Lyr    Cycle <= 150d.
V0417 Lyr    Min II 16.2. P var?
V0418 Lyr    P var. The elements are valid during JD2437100 - 40400.
V0423 Lyr    Min II 15.5. P var?
V0424 Lyr    Blazhko effect?
V0428 Lyr    Min II 14.3. Apsidal motion?
V0429 Lyr    Min II 14.8?
V0431 Lyr    Min II 15.1.
V0435 Lyr    Possibly ew with twice longer P. P may be spurious.
V0462 Lyr    P var? The elements are valid during JD2439913 - 40007.
V0467 Lyr    Min II 12.9. JD2415288 - 43287; the elements
V0467 Lyr    are valid during JD2415288 - 43287; large scatter
V0467 Lyr    on the light curve. According to [09412], during
V0467 Lyr    JD2443424 - 44165 the light variation range is 12.4m -
V0467 Lyr    12.6m pg, the elements are not valid.
V0470 Lyr    U = 0.40", p = 7deg. P1 = 738.6s, P2 = 557.4s, P3 = 318.0s,
V0470 Lyr    P4 = 291.9s, P5 = 259.1s.
V0473 Lyr    P var, Delta(m) var. According to [09413], P =
V0473 Lyr    1.490795d + 1.22d*10**(-6)*(JD - 2443600)/365.25d.
V0473 Lyr    Cyclic P variations: P alpha = 1178.5d; Pt = 2655d.
V0473 Lyr    Delta(m) varies with the period P alpha; P4 = 1063.5d
V0473 Lyr    may be traced in the variations of Vr.
V0473 Lyr    0.06m <= Delta(m) <= 0.36m.
V0474 Lyr    P2 = 76d.
V0477 Lyr    The central star of planetary nebula Abell 46. Strong
V0477 Lyr    reflection effect. Depths of minima: Min I 1.42m B,
V0477 Lyr    Min II ~0.1m B.
V0531 Lyr    Minima observed only between JD 2448600 and 2448800.
V0550 Lyr    SB, Porb = 1.0309d.
V0591 Lyr    MinII 13.85.
V0592 Lyr    MinII 12.82.
V0604 Lyr    According to [265], P = 11.5791 d.
V0608 Lyr    Called SBG 3268 in [267], in contradiction with the star's coordinates and brightness.
V0609 Lyr    The period in the table is twice that in [267], to justify the suggested classification.
V0627 Lyr    According to [267], P = 3.34154 d.
V0634 Lyr    The coordinates in [266] are wrong.
V0641 Lyr    P = 0.4599d is not excluded.
V0664 Lyr    VB A (A 13.0mV; B 14.5mV, 11", 302deg, 1998).
V0668 Lyr    Multiperiodic.
V0691 Lyr    O'Connell effect.
V0722 Lyr    A post-asymptotic-branch star with non-periodic, sometimes rapid, brightness variations.
V0723 Lyr    Multiperiodic, P2 = 0.0745095d.
alf   Lyr    IR excess.
bet   Lyr    ADS 11745 A (B 8.6m, B7V, 46", 149deg; C 13.0m, 47",
bet   Lyr    248deg). Min II 3.85. P var. Nonlinear terms:
bet   Lyr    +3.883d*10**(-6)*E**2 - 0.10d*10**(-10)*E**3.
bet   Lyr    Light curve shape var.
bet   Lyr    Radio and X-ray source. IR excess.
del 2 Lyr    Open cluster delta**2 Lyr member [02505].
R     Men    Sometimes P = 120d;
R     Men    Sometimes P = 240d.
T     Men    In the Large Magellanic Cloud region; not a member of the
T     Men    Cloud. There is a sguare term in the elements:
T     Men    +8.1d*10**(-6)*E**2.
U     Men    VB A (B 10.4m, 0.6", 71deg, 1935.3). A var
U     Men    (0.8m <= A <= 2.9M). P var. Max = 2416927 + 426.9d*E
U     Men    (JD2415200 - 17400) [00207]; since JD2417400 - see Table.
V     Men    Epoch corresponds to the middle of
V     Men    the light curve ascending branch.
W     Men    The member of the Large Magellanic Cloud.
RR    Men    Min II 12.1.
RS    Men    In the Large Magellanic Cloud region; not
RS    Men    a member of the Cloud.
RT    Men    In the Large Magellanic Cloud region; not a member of
RT    Men    the Cloud.
RU    Men    In the Large Magellanic Cloud region; not a member of
RU    Men    the Cloud.
RV    Men    In the Large Magellanic Cloud region; not a member of
RV    Men    the Cloud.
RW    Men    In the Large Magellanic Cloud region; not a member of
RW    Men    the Cloud.
TU    Men    Porb = 0.1176d [09376]. Superhump
TU    Men    Period Ps = 0.12625d [04772].
TY    Men    Min II 8.47; d I = 0.00P, d II = 0.07P.
TY    Men    Shape of the light curve varies.
TZ    Men    Min II 6.36.
UX    Men    Min II 9.47; Min II - Min I = 0.50045P.
UX    Men    One of the components may be a physical variable.
WY    Men    In the region of the NGC 1841 globular cluster; not a
WY    Men    member of the cluster. In the halo of the magellanic
WY    Men    clouds system.
WZ    Men    In the region of the NGC 1841 globular cluster, not a
WZ    Men    member of the cluster. In the halo of the Magellanic
WZ    Men    Clouds system.
XX    Men    In the region of the NGC 1841 globular cluster, not a
XX    Men    member of the cluster. In the halo of the Magellanic
XX    Men    Clouds system.
XY    Men    In the Large Magellanic Cloud region; not a member of the
XY    Men    Cloud. Min II 10.88; dI = 0.05P; dII = 0.00P.
XZ    Men    There are there oscillations simultaneously: P1 = 0.1083d
XZ    Men    (A1 = 0.0094m B), P2 = 0.0855d (A2 = 0.0082m B),
XZ    Men    P3 = 0.0955d (A3 = 0.0058m B); P2/P1 = 0.789.
AN    Men    Type RRC: is also possible.
AT    Men    LMC non-member.
AU    Men    LMC non-member.
BB    Men    Min II = 11.80. P varies. dP/dt = +0.21 x 10^(-5) d/yr.
BC    Men    VB B (A 7.54m; AB 16", 260deg, 2000).
iot   Men    Min II 6.05.
R     Mic    P var. Max = 2413373 + 138.60d*E (JD2413300 - 29600)
R     Mic    [00458]; Max = 2432745 + 137.43d*E (JD2429600 - 34700);
R     Mic    Max = 2435091 + 140.84d*E (JD2434700 - 37800);
R     Mic    since JD2437800 - see Table.
S     Mic    P var. Max = 2413499 + 214.5d*E (JD2413500 - 15900) [00458];
S     Mic    Max = 2432102 + 208.23d*E (JD2422700 - 32200);
S     Mic    since JD2432200 - see Table.
U     Mic    OH, H2O emission.
V     Mic    OH, H20 emission.
Y     Mic    Mean brightness varies.
Z     Mic    (k - b)2 = 0.12; Delta(S) = 4.
RR    Mic    [A/H] = -1.4. P var. Max = 2433032.96 + 31.78175d*E
RR    Mic    (JD2415000 - 35300) [02747]; since JD2443600 - see Table.
RY    Mic    P var? Elements given in the Table represent observations
RY    Mic    in the interval JD2436100 - 40210.
RY    Mic    According to [00085] Max = 2428670 + 190d*E.
RZ    Mic    Min II 11.2.
TV    Mic    Min II 12.4.
UZ    Mic    Min II 12.4.
VW    Mic    In the interval JD2436600 - 840)
VW    Mic    Max = 2436807.248 + 0.35620d*E. Since JD2442600 - see
VW    Mic    Table.
WY    Mic    P = 0.511427d? [00001].
XZ    Mic    In the interval JD2436670 - 840 Max =
XZ    Mic    2436731.480 + 0.449208d*E. Since JD2442630 - see Table.
ZZ    Mic    (k - b)2 = 021; Delta(S) = 0. P var? Max = 2437192.3131 +
ZZ    Mic    0.0671786d*E (JD2437180 - 460) [04308];
ZZ    Mic    Max = 2439320.2162 + 0.0671575d*E (JD2439320 - 340)
ZZ    Mic    [05683]; since JD2440440 - see Table.
ZZ    Mic    Further period increase is possible [09380]. According
ZZ    Mic    to [07985] there are two simultaneous oscillations with the
ZZ    Mic    periods P1 and P2: P1 = 0.0654d, P2 = 0.0513d.
ZZ    Mic    P2/P1 = 0.784; A2(U) = 0.25 A1(U).
AE    Mic    In the interval JD2436670 - 840 Max =
AE    Mic    2436728.470 + 0.324142d*E. Since JD2442630 - see Table.
AH    Mic    Min II 13.6.
AT    Mic    VB (A 10.83m V, M 4.5Ve; B 10.9m V, M 4.5Ve; a =
AT    Mic    6.40", P = 675 yr, e = 0.60 [09381].
AT    Mic    mu alpha = + 0.0216s, mu delta = -0.331" (mu, Vr,
AT    Mic    pi - common with AU Mic).
AT    Mic    Unusually high freguency of flares
AT    Mic    allows to suppose that both components are variable.
AT    Mic    The range of combined brightness variation of the
AT    Mic    system is given in the Table.
AU    Mic    mu alpha = +0.0212S, mu delta = -0.348" (mu, pi,
AU    Mic    Vr - common with AT Mic). SB? 0.20P <= M - m <= 0.55P.
AU    Mic    There are periodical light variations and also flares with
AU    Mic    A <= 0.5m U [08601].
AW    Mic    mu alpha = +0.0077s, mu delta = -0.089".
AW    Mic    Shape of the light curve strongly varies. Multiperiodicity
AW    Mic    is possible.
AX    Mic    mu alpha = -0.2805s, mu delta = -1.152". In
AX    Mic    minimum brightness B - V = +1.42, U - B = +1.20.
CZ    Mic    MinII 12.9:.
DE    Mic    MinII 8.00.
R     Mon    Peculiar non-stellar object at the apex of the reflection
R     Mon    variable [09396] cometary nebula NGC 2261. Probably young
R     Mon    star surrounded by dust cloud. Light curve in [09394].
S     Mon    In the open star cluster
S     Mon    NGC 2264. VB A (B 8.2m, 2.9", 213deg; 9.9m, 16.6", 14deg.)
T     Mon    SB (Porb> = 70 yr [09397]). [A/H] = 0.3.
T     Mon    There is a sguare term in the elements given in the
T     Mon    Table: +5.34d*10**(-6)*E**2.
T     Mon    Deviations from the parabola in the O - C, E diagram
T     Mon    have a wave-like trend. If this wave is attributed to
T     Mon    the light-time effect, Porb = 100 years.
T     Mon    The observations are also satisfied by the following
T     Mon    system of linear elements: Max = 2412874.56 + 27.0093d*E
T     Mon    (JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E
T     Mon    (JD2415250 - 27150); since JD2427150 -
T     Mon    Max = 2436137.090 + 27.0205d*E [02392].
U     Mon    P var. Min = 2408897 + 92.26d*E (JD2408800 - 36210) [00368];
U     Mon    since JD2437300 - see Table.
U     Mon    Mean magnitude varies with the period 2320d [00657].
U     Mon    Spectrum investigation [02226].
V     Mon    P var. Max = 2412172 + 334.5d*E (JD2412000 - 23500) [00458];
V     Mon    Max = 2427870 + 332.5d*E (JD2423500 - 28200);
V     Mon    Max = 2429904 + 342.0d*E (JD2428200 - 30800);
V     Mon    Max = 2439570 + 331.6d*E (JD2430800 - 41225);
V     Mon    since JD2441225 - see Table.
X     Mon    P var. Max = 2415078 + 154.0d*E (JD2415000 - 18800);
X     Mon    Max = 2419758 + 149.6d*E (JD2419700 - 21000);
X     Mon    Max = 2421136 + 155.0d*E (JD2421000 - 24600);
X     Mon    Max = 2424673 + 169d*E (JD2424600 - 25600);
X     Mon    Max = 2425644 + 155.6d*E (JD2425600 - 26800);
X     Mon    Max = 2427028 + 150.7d*E (JD2427000 - 28000) [00458];
X     Mon    Max = 2429521 + 155.8d*E (JD2428000 - 36300);
X     Mon    Max = 2438846 + 145.3d*E (JD2437800 - 38900); since
X     Mon    JD2440800 - see Table. The amplitude strongly varies;
X     Mon    sometimes irregular light variations are observed.
Y     Mon    P var. Max = 2415792 + 228.6d*E (JD2415300 - 19700);
Y     Mon    Max = 2419928 + 227.4d*E (JD2419700 - 24300) [00458];
Y     Mon    Max = 2432647 + 233.3d*E (JD2424300 - 32900);
Y     Mon    since JD2432900 - see Table.
RR    Mon    P var. Max = 2417476 + 384.5d*E (JD2417400 - 19600) [00458];
RR    Mon    since JD2419600 - see Table.
RU    Mon    Min II 11.06; D II var: 0.06P <= DII <= 0.12P;
RU    Mon    Min II - Min I var: 0.25P < = Min II - Min I <= 0.75P.
RU    Mon    P var. In the interval JD2429100 - 38409 Min I =
RU    Mon    2418357.0140; 3.5846794d(E - 406) - 0.429d cos alpha +
RU    Mon    0.06d*sin(2alpha) + 0.010d*cos(3alpha) +
RU    Mon    0.003d*sin(4alpha), MinII = 2418355.2220 +
RU    Mon    3.5846794d(E - 406) + 0.429d cos alpha +
RU    Mon    0.060D*sin(2alpha) - 0.010d cos*3alpha +
RU    Mon    0.003d*sin(4alpha) (JD2416900 - 29100);
RU    Mon    Min I = 2429641.567 + 3.5846391d*(E - 3554) -
RU    Mon    0.429d*cos(alpha) + 0.060d*sin(2alpha) + 0.010d*cos(3alpha) +
RU    Mon    0.003d*sin(4alpha),
RU    Mon    Min II = 2429639.775 + 3.5846391d(E - 3554) +
RU    Mon    0.429d*cos(alpha) + 0.060d*sin(2alpha) -
RU    Mon    0.010d*cos(3alpha) + 0.003d*sin(4alpha), where alpha =
RU    Mon    0.01245deg(E - 406) [03445].
RU    Mon    The epochs E are being calculated for Min I from JD hel.
RU    Mon    2416901.205, and for Min II - from JD hel. 2416900.248.
RU    Mon    In the interval JD2438409 - 41743
RU    Mon    Min I = 2438409.6045 + 3.584586d(E - 6000) -
RU    Mon    0.4290d*cos(alpha) + 0.0620d*sin(2alpha) +
RU    Mon    0.0107d*cos(3alpha) + 0.0026d*sin(4alpha) -
RU    Mon    0.00036d cos 5alpha, Min II = 2438407.8122 +
RU    Mon    3.584586d(E - 6000) + 0.4290d cos alpha +
RU    Mon    0.0620d*sin(2alpha) - 0.0107d*cos(3alpha) +
RU    Mon    0.0026d*sin(4alpha) + 0.00036d*cos(5alpha),
RU    Mon    where alpha = 0.012385deg(E - 406) [07987].
RU    Mon    since JD2441743 - Min I = 2441743.2633 +
RU    Mon    3.584670d(E - 6930) - 0.4336d cos alpha +
RU    Mon    0.0634d*sin(2alpha) + 0.0111d*cos(3alpha) +
RU    Mon    0.0021d*sin(4alpha), Min II = 2441741.4710 +
RU    Mon    3.584689d(E - 6930) + 0.4336d cos alpha +
RU    Mon    0.0634d*sin(2alpha) - 0.0111d*cos(3alpha) +
RU    Mon    0.0021d*sin(4alpha), where alpha = 70.6deg +
RU    Mon    0.0114deg(E - 6094) [09546]. Linear elements for Min I
RU    Mon    epochs in 1973 - 1990 are given in the Table.
RU    Mon    Corresponding elements for Min II epochs are:
RU    Mon    Min II = 2441741.575 + 3.584567d*E. E = 0.38.
RU    Mon    Apsidal motion period is 285 years.
RV    Mon    Mean brightness varies with P = 1047d.
RW    Mon    Min II 9.45; d I = 0.027P, d II = 0.023P. P var.
RW    Mon    Min I = 2417943.687 + 1.9061012d*E (JD2417940 - 32900)
RW    Mon    [03450]; since JD2432900 - see Table.
RX    Mon    P var. Max = 2418980 + 343.2d*E (JD2416200 -
RX    Mon    19000); Max = 2423097 + 338.9d*E (JD2422000 -
RX    Mon    28500); since JD2428500 - see Table.
RY    Mon    VB A (B 12.29M, 28").
SS    Mon    In the region of the open cluster NGC 2264.
SU    Mon    S 5/7 - S 6/7. P var: 69d (JD2416700 - 19100); 203.5d
SU    Mon    (JD2420100 - 22920); 69d (JD2423000 - 30100).
SU    Mon    In the intervals JD2423000 - 520 - const (11.5m),
SU    Mon    JD2424820 - 980 - const (11.8m).
SV    Mon    [A/H] = 0.2. P var. Max = 2419041.805 + 15.230721d*E
SV    Mon    (JD2412000 - 22000) [00025]; Max = 2422651.931 +
SV    Mon    15.23256d*E (JD2422600 - 23850) [09400]; Max =
SV    Mon    2424571.60 + 15.2513d*E (JD2423850 - 24600);
SV    Mon    Max = 2434045.326 + 15.2304d*E (JD2424600 - 34100);
SV    Mon    since JD2433000 - see Table.
SX    Mon    Mean brightness varies with P = 1100d.
SZ    Mon    VB A (B 11m - 12m, 10" [09401]). Min II 10.55. P var.
SZ    Mon    Min I = 2426357.1 + 32.760d*E (JD2422000 - 26400);
SZ    Mon    Min I = 2427861.2 + 32.708d*E (JD2426750 - 32000);
SZ    Mon    since JD2432800 - see Table.
SZ    Mon    Shape of the light curve varies. Heights of maxima and
SZ    Mon    depths of minima are constant.
TU    Mon    Min II 9.1.
TV    Mon    In the region of the open star cluster NGC 2237.
TW    Mon    Wachmann [03453] assigns the variable to the RRab
TW    Mon    type with the elements Max = 2433001.371 + 0.8743887*E,
TW    Mon    but notes a considerable dispersion of the points around
TW    Mon    the mean light curve obtained with this period. As the
TW    Mon    periods by Hessner (PH) and Wachmann (PW) are mutually
TW    Mon    related (1/PW ~1/PH + 1) it is more probable on account of
TW    Mon    the above mentioned circumstance that the variable belongs
TW    Mon    to cepheids.
TX    Mon    [A/H] = -0.3.
UV    Mon    The form of the light curve being unusual for RR Lyr type
UV    Mon    variables (Max II 13.5 at the phase 0.39P, Min II 13.8
UV    Mon    at the phase 0.22P), the period may be doubtful,
UV    Mon    though it was found independently by two investigators
UV    Mon    [00380, 03453].
UX    Mon    Min II 8.52; dI = 0.044P. P var?
UX    Mon    Brightness in maximum varies with the amplitude up to 0.2m.
VV    Mon    Min II 9.55; dI = dII = 0.07P.
VV    Mon    There is a square term in the elements given in the Table:
VV    Mon    -0.12d*10**(-7)*E**2.
VW    Mon    P var. Max = 2425243.40 + 0.6041350d*E (JD2414700 -
VW    Mon    30700); since JD2430700 - see Table.
VW    Mon    In [00386, 05448] And other previous works the spurious
VW    Mon    period value 1.532d is being accepted suggesting the
VW    Mon    curious nature of the variable. Serious observations are
VW    Mon    necessary to select the true value of the period.
VX    Mon    Depth of Min II 0.07m.
VY    Mon    In the region of the nebula IC 446.
XX    Mon    [A/H] = -0.2.
XZ    Mon    Min II 13.6; d = 0.02P:.
AA    Mon    [A/H] = -0.9. P var. Max = 2430788.266 + 3.938052d*E
AA    Mon    (JD2425300 - 34800) [03453]; since JD2434800 - see Table.
AC    Mon    In the region of the open cluster NGC 2323.
AK    Mon    P var. Max = 2425279 + 319.2d*E (JD2425200 - 28000); since
AK    Mon    JD2428000 - see Table.
AN    Mon    Min II 11.7:; d = 0.027P.
AO    Mon    Min II 10.16; DII = 0.14P; Min II - Min I = 0.4933P. P var.
AO    Mon    Min I = 2426735.333 + 1.884758d*E (JD2426700 - 40000);
AO    Mon    since JD2440000 - see Table.
AQ    Mon    Min II 10.9; DII = 0.05P; dI = 0.014P.
AR    Mon    Min II 9.03; d = 0.011P.
AR    Mon    There is a square term in the elements given in the Table:
AR    Mon    -1.22d*10**(-6)*E**2.
AU    Mon    Min II 8.2:. Shape of the light curve varies.
AU    Mon    Brightness in maximum varies periodically with the
AU    Mon    amplitude 0.2m: Max = 2443105 + 411d*E; M - m = 0.5P.
AV    Mon    Depth of Min II 0.04m.
AW    Mon    P var. Min = 2425649.053 + 20.797d*E (JD2425500 -
AW    Mon    26400) [09408]; Min = 2426439.340 + 20.81905d*E
AW    Mon    (JD2426400 - 35900) [00511]; since JD2435900 - see Table.
AX    Mon    Binary system with an envelope and gaseous streams.
AX    Mon    Porb = 232.60d [06103]. Spectrum investigation [09411].
AX    Mon    Epoch of Min brightness preceeding the moment of
AX    Mon    conjunction for 0.25p is given in the Table; A = 0.4m U.
AX    Mon    Besides periodical variations, there are rapid light
AX    Mon    fluctuations up to 0.1m.
BB    Mon    Depth of Min II 0.04m.
BC    Mon    P var. Max = 2421240 + 275.8d*E (JD2421200 -
BC    Mon    25960); Max = 2428880 + 267.2d*E (JD2425960 -
BC    Mon    30000); since JD2430000 - see Table.
BE    Mon    Delta(S) = 0.
BH    Mon    d = 0.01p:.
BM    Mon    Min II 12.3. According to [09415], apsidal motion is
BM    Mon    possible.
BO    Mon    Min II 10.1. P var. Min I = 2428211.596 + 2.2251753d*E
BO    Mon    (JD2415000 - 36000) [00007]; since JD2436000 - see Table.
BP    Mon    P var?
BP    Mon    Elements given in the Table are valid in the interval
BP    Mon    JD2425600 - 29700.
BT    Mon    VB A (B 16.0m, 10", 0deg).
BT    Mon    After the outburst in 1939 the brightness varies in the
BT    Mon    range 16.0m - 18.7m with the elements: Min =
BT    Mon    2443491.7155 + 0.3338141d*E; D = 0.20p, 0 <= d < = 0.03p.
BT    Mon    Before the outburst in 1939, according to [09417],
BT    Mon    the following elements were valid: Min = 2429500.207 +
BT    Mon    0.3338010d*E. Emission nebula with the radius of 3.8"
BT    Mon    was discovered in 1981 around the nova [09148].
BX    Mon    Usually was considered as mira type variable
BX    Mon    [09421]. In the Table the epoch of light maximum and
BX    Mon    the period are given according to [09419]. According
BX    Mon    to [09420] the Balmer emission lines originate in the
BX    Mon    nebulosity surrounding the symbiotic system and are
BX    Mon    excited by the hot component, and light variations
BX    Mon    are due to the orbital motion in the system.
BZ    Mon    d = 0.030P. In the region of the open cluster CR 106.
CC    Mon    In the region of the open cluster CR 106.
CD    Mon    P var. Max = 2427704 + 273.8d*E (JD2427400 - 30400); since
CD    Mon    JD2430400 - see Table.
CE    Mon    Min II 14.2.
CF    Mon    Min II 13.7; d = 0.02P:.
CH    Mon    d = 0.030P.
CS    Mon    VB A (B 13m, 9", 0deg).
CT    Mon    In the region of the open cluster NGC 2244.
CU    Mon    [A/H] = -0.2.
CV    Mon    In the centre of an anonymous open cluster.
CV    Mon    VB A (B 13.76m, 10", 270deg; C 13.72m, 14", 270deg).
CV    Mon    P var. Max = 2429805.142 + 5.378782d*E (JD2429360 -
CV    Mon    36000); since JD2436000 - see Table.
DD    Mon    Min II 11.3.
DF    Mon    The chart in [05285] is wrong, the star observed was
DF    Mon    not DF Mon.
DN    Mon    Min II 13.9.
DR    Mon    In the region of the open cluster Cr 106.
DT    Mon    P var. Max = 2425324 + 345d*E (JD2425300 - 28200)
DT    Mon    In the interval JD2429250 - 37700 there were cycles 119d,
DT    Mon    230d, 350d.
DW    Mon    In the region of the open cluster NGC 2286.
EE    Mon    P var. Max = 2425300.42 + 4.80776d*E (JD2425300 -
EE    Mon    27720); since JD2427720 - see Table.
EH    Mon    d = 0.023P.
EK    Mon    P var. Max = 2425302.59 + 3.95773d*E (JD2425200 -
EK    Mon    33000) [00387]; since JD2433000 - see Table.
EP    Mon    d = 0.026P.
ES    Mon    d = 0.02P.
EW    Mon    Min II 14.2.
FH    Mon    Depth of Min II 0.04m.
FP    Mon    In the region of the open cluster NGC 2353.
FS    Mon    Min II 11.2.
FU    Mon    S 6.5/7.5.
FW    Mon    d = 0.016P. Depth of Min II 0.04m.
FX    Mon    OH emission.
FZ    Mon    The elements should be checked.
GH    Mon    Min II 13.1.
GP    Mon    In the region of the open cluster NGC 2264.
GQ    Mon    In the region of the open cluster NGC 2264.
GR    Mon    In the region of the open cluster NGC 2264.
GU    Mon    Min II 12.5.
GV    Mon    Depth of Min II 0.04m.
GX    Mon    OH, H2O, SIO maser.
HI    Mon    Min II 9.9.
HM    Mon    Min II 13.6. P var. Min I = 2430110.1948 + 0.40765737d*E
HM    Mon    (JD2429600 - 35400) [05285]; since JD2435400 - see Table.
HO    Mon    d = 0.03P.
HP    Mon    d = 0.04P:.
HR    Mon    Depth of Min II 0.03m.
HY    Mon    Min II 12.4.
IL    Mon    d = 0.03P.
IM    Mon    Min II 6.47.
IO    Mon    In the region of the open cluster NGC 2264.
IP    Mon    In the region of the open cluster NGC 2264.
IQ    Mon    In the region of the open cluster NGC 2264.
IR    Mon    P var?
IS    Mon    Depth of Min II 0.05m.
IX    Mon    Min II 12.8.
IZ    Mon    Min II 12.0.
KU    Mon    In the region of the open cluster NGC 2264.
KV    Mon    In the region of the open cluster NGC 2264.
KW    Mon    In the region of the open cluster NGC 2264.
KX    Mon    In the region of the open cluster NGC 2264.
KY    Mon    In the region of the open cluster NGC 2264.
KZ    Mon    In the region of the open cluster NGC 2264.
LL    Mon    In the region of the open cluster NGC 2264.
LM    Mon    In the region of the open cluster NGC 2264.
LN    Mon    In the region of the open cluster NGC 2264.
LO    Mon    In the region of the open cluster NGC 2264.
LP    Mon    In the region of the open cluster NGC 2264.
LQ    Mon    In the region of the open cluster NGC 2264.
LR    Mon    In the region of the open cluster NGC 2264.
LS    Mon    In the region of the open cluster NGC 2264.
LT    Mon    In the region of the open cluster NGC 2264.
LU    Mon    In the region of the open cluster NGC 2264.
LV    Mon    In the region of the open cluster NGC 2264.
LW    Mon    In the region of the open cluster NGC 2264.
LX    Mon    In the region of the open cluster NGC 2264.
LY    Mon    In the region of the open cluster NGC 2264.
LZ    Mon    In the region of the open cluster NGC 2264.
MM    Mon    In the region of the open cluster NGC 2264.
MN    Mon    In the region of the open cluster NGC 2264.
MO    Mon    VB A (B 20m, 10", 356deg); in the region of the
MO    Mon    open cluster NGC 2264.
MP    Mon    In the region of the open cluster NGC 2264.
MQ    Mon    In the region of the open cluster NGC 2264.
MX    Mon    Min II 11.7.
NN    Mon    Min II 12.9.
NS    Mon    Min II 11.1.
NT    Mon    In the region of the open cluster NGC 2264.
NU    Mon    In the region of the open cluster NGC 2264.
NV    Mon    In the region of the open cluster NGC 2264.
NW    Mon    In the region of the open cluster NGC 2264.
NX    Mon    In the region of the open cluster NGC 2264.
NY    Mon    In the region of the open cluster NGC 2264.
NZ    Mon    In the region of the open cluster NGC 2264.
OO    Mon    In the region of the open cluster NGC 2264.
OP    Mon    In the region of the open cluster NGC 2264.
OQ    Mon    In the region of the open cluster NGC 2264.
OR    Mon    In the region of the open cluster NGC 2264.
OS    Mon    In the region of the open cluster NGC 2264.
OT    Mon    In the region of the open cluster NGC 2264.
OU    Mon    In the region of the open cluster NGC 2264.
OV    Mon    In the region of the open cluster NGC 2264.
OW    Mon    In the region of the open cluster NGC 2264.
OX    Mon    VB A (B 15m, 7", 35deg); in the region of the open
OX    Mon    cluster NGC 2264.
OY    Mon    In the region of the open cluster NGC 2264.
OZ    Mon    In the region of the open cluster NGC 2264.
PP    Mon    In the region of the open cluster NGC 2264.
PQ    Mon    In the region of the open cluster NGC 2264.
PR    Mon    The elements should be checked.
PT    Mon    In the region of the open cluster NGC 2264.
PU    Mon    In the region of the open cluster NGC 2264.
PV    Mon    In the region of the open cluster NGC 2264.
PW    Mon    In the region of the open cluster NGC 2264.
PX    Mon    In the region of the open cluster NGC 2264.
PY    Mon    In the region of the open cluster NGC 2264.
QR    Mon    290d <= P <= 400d. Depth of Min varies by
QR    Mon    0.9m with the period about 2000d.
QT    Mon    In the region of the open cluster NGC 2264.
QU    Mon    In the region of the open cluster NGC 2264.
QV    Mon    In the region of the open cluster NGC 2264.
QW    Mon    In the region of the open cluster NGC 2264.
QX    Mon    In the region of the open cluster NGC 2264.
QY    Mon    In the region of the open cluster NGC 2264.
QZ    Mon    In the region of the open cluster NGC 2264.
V0335 Mon    In the region of the open cluster NGC 2264.
V0336 Mon    In the region of the open cluster NGC 2264.
V0337 Mon    In the region of the open cluster NGC 2264.
V0338 Mon    In the region of the open cluster NGC 2264.
V0339 Mon    In the region of the open cluster NGC 2264.
V0340 Mon    In the region of the open cluster NGC 2264.
V0341 Mon    In the region of the open cluster NGC 2264.
V0342 Mon    In the region of the open cluster NGC 2264.
V0343 Mon    In the region of the open cluster NGC 2264.
V0344 Mon    In the region of the open cluster NGC 2264.
V0345 Mon    In the region of the open cluster NGC 2264.
V0346 Mon    In the region of the open cluster NGC 2264.
V0347 Mon    VB A (B 20m, 12", 120deg); in the region of the open
V0347 Mon    cluster NGC 2264.
V0348 Mon    In the region of the open cluster NGC 2264.
V0349 Mon    In the region of the open cluster NGC 2264.
V0350 Mon    In the region of the open cluster NGC 2264.
V0351 Mon    In the region of the open cluster NGC 2264.
V0352 Mon    In the region of the open cluster NGC 2264.
V0353 Mon    In the region of the open cluster NGC 2264.
V0354 Mon    In the region of the open cluster NGC 2264.
V0355 Mon    In the region of the open cluster NGC 2264.
V0356 Mon    VB (3", 78deg); in the region of the open cluster
V0356 Mon    NGC 2264.
V0357 Mon    In the region of the open cluster NGC 2264.
V0358 Mon    In the region of the open cluster NGC 2264.
V0359 Mon    In the region of the open cluster NGC 2264.
V0360 Mon    In the region of the open cluster NGC 2264.
V0361 Mon    In the region of the open cluster NGC 2264.
V0362 Mon    In the region of the open cluster NGC 2264.
V0363 Mon    In the region of the open cluster NGC 2264.
V0364 Mon    In the region of the open cluster NGC 2264.
V0365 Mon    VB B (A = V591 Mon, B 7", 135deg); in the region of the
V0365 Mon    open cluster NGC 2264.
V0366 Mon    In the region of the open cluster NGC 2264.
V0367 Mon    In the region of the open cluster NGC 2264.
V0368 Mon    VB (9", 252deg); in the region of the open cluster
V0368 Mon    NGC 2264.
V0369 Mon    VB (11", 264deg); in the region of the open cluster
V0369 Mon    NGC 2264.
V0370 Mon    VB (8", 97deg); in the region of the open cluster
V0370 Mon    NGC 2264.
V0371 Mon    In the region of the open cluster NGC 2264.
V0372 Mon    SC 7/7.5.
V0373 Mon    In the region of the open cluster NGC 2264.
V0379 Mon    d = 0.015P:.
V0380 Mon    Min II 12.9; P = 1.98904166d?
V0383 Mon    Min II 15.2.
V0384 Mon    Min II 13.0.
V0389 Mon    Min II 14.9.
V0393 Mon    Min II 14.3.
V0394 Mon    d = 0.02P; depth of Min II 0.04m.
V0395 Mon    d = 0.03P.
V0396 Mon    Min II 13.5.
V0397 Mon    Min II 11.9.
V0398 Mon    In the region of the open cluster NGC 2264.
V0399 Mon    In the region of the open cluster NGC 2264.
V0400 Mon    In the region of the open cluster NGC 2264.
V0401 Mon    In the region of the open cluster NGC 2264.
V0402 Mon    In the region of the open cluster NGC 2264.
V0403 Mon    In the region of the open cluster NGC 2264.
V0404 Mon    d = 0.02P:.
V0405 Mon    In the region of the open cluster NGC 2264.
V0406 Mon    In the region of the open cluster NGC 2264.
V0407 Mon    In the region of the open cluster NGC 2264.
V0408 Mon    In the region of the open cluster NGC 2264.
V0409 Mon    In the region of the open cluster NGC 2264.
V0410 Mon    In the region of the open cluster NGC 2264.
V0411 Mon    In the region of the open cluster NGC 2264.
V0412 Mon    In the region of the open cluster NGC 2264.
V0413 Mon    In the region of the open cluster NGC 2264.
V0414 Mon    In the region of the open cluster NGC 2264.
V0415 Mon    In the region of the open cluster NGC 2264.
V0416 Mon    In the region of the open cluster NGC 2264.
V0417 Mon    In the region of the open cluster NGC 2264.
V0418 Mon    In the region of the open cluster NGC 2264.
V0419 Mon    In the region of the open cluster NGC 2264.
V0420 Mon    In the region of the open cluster NGC 2264.
V0421 Mon    In the region of the open cluster NGC 2264.
V0422 Mon    In the region of the open cluster NGC 2264.
V0423 Mon    In the region of the open cluster NGC 2264.
V0424 Mon    In the region of the open cluster NGC 2264.
V0425 Mon    In the region of the open cluster NGC 2264.
V0426 Mon    VB A (B = NSV 3125 17.0m, 6", 117deg); in the region of
V0426 Mon    the open cluster NGC 2264.
V0427 Mon    In the region of the open cluster NGC 2264.
V0428 Mon    In the region of the open cluster NGC 2264.
V0429 Mon    In the region of the open cluster NGC 2264.
V0430 Mon    In the region of the open cluster NGC 2264.
V0431 Mon    In the region of the open cluster NGC 2264.
V0432 Mon    In the region of the open cluster NGC 2264.
V0433 Mon    In the region of the open cluster NGC 2264.
V0434 Mon    In the region of the open cluster NGC 2264.
V0435 Mon    In the region of the open cluster NGC 2264.
V0436 Mon    In the region of the open cluster NGC 2264.
V0437 Mon    In the region of the open cluster NGC 2264.
V0438 Mon    In the region of the open cluster NGC 2264.
V0439 Mon    In the region of the open cluster NGC 2264.
V0440 Mon    In the region of the open cluster NGC 2264.
V0441 Mon    In the region of the open cluster NGC 2264.
V0442 Mon    Min II 11.6.
V0443 Mon    In the region of the open cluster NGC 2264.
V0444 Mon    In the region of the open cluster NGC 2264.
V0445 Mon    Min II 11.3.
V0446 Mon    [A/H] = -0.7.
V0447 Mon    [A/H] = -1.4.
V0448 Mon    Min II 9.8.
V0449 Mon    d = 0.02P.
V0450 Mon    Min II 12.6.
V0451 Mon    Min II 14.7.
V0452 Mon    Min II 12.7; d = 0.02P.
V0453 Mon    Min II 11.8.
V0454 Mon    Min II 12.2.
V0455 Mon    Min II 15.3.
V0456 Mon    Min II 13.7.
V0457 Mon    Min II 14.3; d = 0.03P:.
V0458 Mon    Min II 13.8.
V0459 Mon    Min II 14.7.
V0460 Mon    Min II 10.7.
V0463 Mon    d = 0.03P; P = 2.2476768d?
V0464 Mon    Min II 12.3.
V0465 Mon    P var. Max = 2429642.44 + 2.71341d*E (JD2425600 -
V0465 Mon    30800) [03551]; Max = 2431845.65 + 2.713212d*E
V0465 Mon    (JD2430000 - 35200) [03453]; Max = 2435541.315 +
V0465 Mon    2.713668d*E (JD2435200 - 41600); since JD2441600 - see
V0465 Mon    Table.
V0466 Mon    VB A (B 15m, 135deg).
V0474 Mon    (k - b)2 = 0.32. Blazhko effect:
V0474 Mon    Max(O - C) = 2441664.962 + 7.74639d*N; Min(O - C) =
V0474 Mon    2441669.569 + 7.74639d*N; 0.03m <= A <= 0.37m;
V0474 Mon    -0.02d <= O - C <= +0.03d. Freguency analysis gives
V0474 Mon    three principal oscillations [08669]: P1 = 0.1361258d
V0474 Mon    (A1 = 0.18m), P2 = 0.1337745d (A2 = 0.12m),
V0474 Mon    P3 = 0.1385591d (A3 = 0.04m).
V0478 Mon    In the region of the nebula IC 2169.
V0479 Mon    In the region of the nebula IC 2169.
V0481 Mon    In the region of the nebula IC 2169.
V0482 Mon    In the region of the nebula IC 2169.
V0483 Mon    In the region of the nebula IC 2169.
V0486 Mon    VB A (B 18.4M, 6"). In the region of the nebula NGC 2245.
V0487 Mon    In the region of the nebula NGC 2245.
V0488 Mon    In the region of the nebula NGC 2245.
V0489 Mon    In the region of the nebula NGC 2245.
V0490 Mon    In the region of the nebula NGC 2247.
V0493 Mon    In the region of the open cluster Tr 5.
V0494 Mon    Depth of Min II 0.05m.
V0496 Mon    Min II 12.8.
V0497 Mon    8.9 - 11.8 IR.
V0498 Mon    P = 2.4727818d?
V0500 Mon    In the region of the open cluster NGC 2264.
V0501 Mon    Min II 13.1; Min II - Min I = 0.445P; DII = 0.036P.
V0503 Mon    9.2 - 10.9 IR.
V0505 Mon    Min II 7.55.
V0507 Mon    SB2 (P = 53.781d [09483]); d = 0.015P:.
V0510 Mon    [A/H] = -0.1.
V0513 Mon    Depth of Min II 0.04m.
V0514 Mon    Min II 13.3.
V0515 Mon    Min II 12.7.
V0521 Mon    Min II 10.4.
V0524 Mon    Min II 15.2.
V0526 Mon    P var. Max = 2433304.284 + 2.675208d*E (JD2429300 -
V0526 Mon    35170); since JD2439170 - see Table.
V0527 Mon    Depth of Min II 0.05m.
V0530 Mon    Min II 12.8.
V0532 Mon    Min II 12.8. RRC?
V0535 Mon    P var. Max = 2431846.445 + 0.3328791d*E
V0535 Mon    (JD2429600 - 34060); since JD2434060 - see Table.
V0535 Mon    [Fe/H] = -1.44.
V0539 Mon    In the region of the open cluster NGC 2244.
V0540 Mon    In the region of the nebula IC 446.
V0541 Mon    In the region of the nebula IC 446.
V0542 Mon    In the region of the nebula IC 446.
V0543 Mon    In the region of the open cluster NGC 2244.
V0544 Mon    In the region of the open cluster NGC 2244.
V0545 Mon    In the region of the open cluster NGC 2244.
V0546 Mon    In the region of the open cluster NGC 2244.
V0547 Mon    In the region of the open cluster NGC 2244.
V0548 Mon    In the region of the open cluster NGC 2244.
V0549 Mon    In the region of the open cluster NGC 2244.
V0550 Mon    VB A (B 17.3m, 6", 0deg ); in the region of the open
V0550 Mon    cluster NGC 2244.
V0551 Mon    In the region of the open cluster NGC 2244.
V0552 Mon    In the region of the open cluster NGC 2244.
V0553 Mon    In the region of the open cluster NGC 2244.
V0554 Mon    In the region of the open cluster NGC 2244.
V0555 Mon    In the region of the open cluster NGC 2244.
V0556 Mon    In the region of the open cluster NGC 2244.
V0557 Mon    In the region of the open cluster NGC 2244.
V0560 Mon    Depth of Min II 0.05m.
V0565 Mon    Connected with the diffuse nebula
V0565 Mon    NGC 2313 having diameter of 10" and a faint cometary
V0565 Mon    nebula.
V0569 Mon    VB A (B 10.8m, 6.2", 281deg; C 10.5m, 38.3", 295deg).
V0569 Mon    The range of combined light variation of A and B
V0569 Mon    components is given. According to [08215], P = 0.18d.
V0571 Mon    (k - b)2 = 0.32.
V0571 Mon    Non-radial pulsation with variable periods:
V0571 Mon    P1 = 0.0999081d (A1 = 0.052m), P2 = 0.0749998d
V0571 Mon    (A2 = 0.015m) (JD2440914 - 41692) [07127]; P1 = 0.0894534d
V0571 Mon    (A1 = 0.038m), P2 = 0.15988d (A2 = 0.025m), P3 = 0.106516d
V0571 Mon    (A3 = 0.014m). P4 = 0.26998d (A4 = 0.012m), P5 = 0.15069d
V0571 Mon    (A5 = 0.011m) (JD2441662 - 719) [09450].
V0577 Mon    VB (A 11.3m V, B 14.8m V; a = 0.312", P = 16.60 yr, e =
V0577 Mon    0.38); mu alpha = +0.049S, mu beta = +0.73".
V0577 Mon    Both components are probably variables. The range
V0577 Mon    of combined light variation of the system is given
V0577 Mon    in the Table [06146].
V0578 Mon    In the region of the open cluster NGC 2244.
V0579 Mon    In the region of the open cluster NGC 2264.
V0580 Mon    In the region of the open cluster NGC 2264.
V0581 Mon    In the region of the open cluster NGC 2264.
V0582 Mon    In the region of the open cluster NGC 2264.
V0583 Mon    In the region of the open cluster NGC 2264.
V0584 Mon    In the region of the open cluster NGC 2264.
V0585 Mon    In the region of the open cluster NGC 2264.
V0586 Mon    In the region of the open cluster NGC 2264.
V0588 Mon    In the region of the open cluster NGC 2264.
V0589 Mon    In the region of the open cluster NGC 2264.
V0590 Mon    VB (10", 358deg); in the region of the open cluster
V0590 Mon    NGC 2264.
V0591 Mon    VB A (B = V365 Mon, 7", 135deg); in the region of the open
V0591 Mon    cluster NGC 2264.
V0593 Mon    In the region of the open cluster NGC 2264.
V0594 Mon    In the region of the open cluster NGC 2264.
V0595 Mon    In the region of the open cluster NGC 2264.
V0596 Mon    In the region of the open cluster NGC 2264.
V0597 Mon    In the region of the open cluster NGC 2264.
V0598 Mon    In the region of the open cluster NGC 2264.
V0599 Mon    In the region of the open cluster NGC 2264.
V0600 Mon    In the region of the open cluster NGC 2264.
V0601 Mon    In the region of the open cluster NGC 2264.
V0602 Mon    In the region of the open cluster NGC 2264.
V0603 Mon    In the region of the open cluster NGC 2264.
V0604 Mon    In the region of the open cluster NGC 2264.
V0605 Mon    In the region of the open cluster NGC 2264.
V0606 Mon    In the region of the open cluster NGC 2264.
V0607 Mon    In the region of the open cluster NGC 2264.
V0608 Mon    In the region of the open cluster NGC 2264.
V0609 Mon    In the region of the open cluster NGC 2264.
V0610 Mon    In the region of the open cluster NGC 2264.
V0611 Mon    In the region of the open cluster NGC 2264.
V0612 Mon    In the region of the open cluster NGC 2264.
V0613 Mon    S 3/2.
V0616 Mon    Novalike outbursts were observed in 1917 (Max JD2421540)
V0616 Mon    and in 1975 (Max JD2442646). In quiescent state probably
V0616 Mon    ellipsoidal light variation is observed with P = 0.325d
V0616 Mon    and A = 0.2m [09458], and also slower light variations
V0616 Mon    with P = 7.39d [09459] or 7.8d [09460]. Spectrum description
V0616 Mon    [09461, 09462].
V0624 Mon    In the region of the open cluster Cr 106.
V0628 Mon    In the region of the open cluster NGC 2264.
V0629 Mon    In the region of the open cluster NGC 2264.
V0630 Mon    VB A (B 21m, 3", 300deg); in the region of the open
V0630 Mon    cluster NGC 2264.
V0632 Mon    In the region of the open cluster NGC 2368.
V0637 Mon    Basic oscillation with A1 = 0.05m and elements given in
V0637 Mon    the Table is superimposed by the second one with
V0637 Mon    A2 = 0.02m and the elements: Max = 2443496.1624 +
V0637 Mon    0.19740d*E. Beat period Pb = 6.09d.
V0638 Mon    VB (6.5m, 8.5m; 0.8", 178deg).
V0640 Mon    In the region of the open cluster NGC 2244.
V0640 Mon    Porb = 14.39604d [06103].
V0640 Mon    Irregular light variations.
V0640 Mon    Probably transitional stage from a binary system of
V0640 Mon    O stars to a system of WR type [04107].
V0641 Mon    VB A (B 10.91m, 21.4", 310deg; C 12.46m, 25.8", 285deg).
V0641 Mon    In the region of the open cluster NGC 2264.
V0642 Mon    In the region of the open cluster NGC 2264. Cluster
V0642 Mon    non-member. Epoch of light minimum is
V0642 Mon    given in the Table.
V0645 Mon    Epoch of light minimum is given in the Table.
V0741 Mon    Type ACV: is also possible.
V0750 Mon    In the region of the nebula IC 2177.
V0753 Mon    Type ACV: is also possible.
V0851 Mon    Cluster non-member.
V0852 Mon    The depth of MinII is at least 0.07.
V0853 Mon    MinII 16.05.
V0857 Mon    MinII 15.98.
V0858 Mon    MinII 15.87.
V0859 Mon    MinII 14.50. Cluster non-member?
V0860 Mon    MinII 9.38.
V0861 Mon    MinII 12.7.
V0863 Mon    MinII 9.13.
V0875 Mon    Multiple (A 12.6mV; B 13.4mV, 18", 218deg; C = var, 14.51mV, 10", 101deg; D 15.8mV, 12", 168deg, 1990). The tabulated variability range could be influenced by the companions.
V0878 Mon    O'Connell effect.
V0879 Mon    VB (A 8.4m, B 10.4m, 7", 265deg, 1999).
V0880 Mon    VB A (A 8.7m; B 9.9m, 14", 300deg, 1991). Combined magnitudes are tabulated.
V0898 Mon    VB A (B 15.0mpg, 19", 173deg, 1999).
V0900 Mon    Min II = 12.65.
V0901 Mon    The tabulated light elements are for the fundamental mode. First overtone: Max = 2453724.711 + 1.61404d x E.
V0902 Mon    Several longer period aliases are also possible.
V0903 Mon    Min II = 12.80.
V0904 Mon    Min II = 12.68.
V0906 Mon    Min II = 10.82.
V0907 Mon    Min II = 10.57.
V0908 Mon    Min II = 11.54.
V0909 Mon    Min II = 10.63.
V0910 Mon    Min II = 11.39.
V0912 Mon    VB A (B 14.4m, 3"s).
V0915 Mon    Min II = 11.15.
V0917 Mon    Min II = 9.93.
V0919 Mon    Min II = 11.7.
V0920 Mon    Min II = 7.48. VB AB (A 7.74m, A2:V:m, SB, Porb = 6.7663d; B 9.18m, G8IIIe, SB, Porb = 4.4813d; AB 0.9", 37deg, 1995). Component A varies.
V0922 Mon    Min II = 11.38.
V0925 Mon    Min II = 8.52.
V0927 Mon    Min II = 11.16.
V0929 Mon    Min II = 13.7.
V0930 Mon    Min II = 8.40.
V0931 Mon    VB AB (A 10.49m; B 11.10m, 3.3", 282deg, 1999).
V0934 Mon    Min II = 13.4.
V0935 Mon    Min II = 9.9. Min II - MinI = 0.78P.
V0936 Mon    Min II = 14.2.
V0937 Mon    Min II = 8.84. Light elements for eclipses are tabulated. Pulsations with P = 0.110480d and amplitude about 0.08m.
V0938 Mon    Min II = 15.0 :.
V0948 Mon    Min II = 13.7.
V0953 Mon    Min II = 14.4. Type RRC with a twice shorter period is not excluded.
S     Mus    Marked on the chart for BO Mus. Max II = Max I,
S     Mus    Phase (Max II) = 0.15P. P var? SB 1 (Porb = 506.4d).
T     Mus    P2 = 1021d.
V     Mus    In the Coal Sack region.
RV    Mus    P = 128d: is possible.
RW    Mus    P = 130d: is possible.
RY    Mus    V1 (NGC 4833).
RZ    Mus    V2 (NGC 4833). Cluster non-member.
SY    Mus    Min II 11.2; Min I - Min II = 170d.
SY    Mus    Elements for Min I of quasiperiodic variations observed
SY    Mus    during JD2434910 - 41510 are given. Radio source.
TU    Mus    Min II 8.65. P var. Min I = 2424260.396 + 1.38728d*E
TU    Mus    (JD2423900 - 29300) [00039]; during JD2437380 - 41900 - see
TU    Mus    Table. The light curve shape var.
TV    Mus    Min II 11.3.
TW    Mus    Min II 12.4.
TZ    Mus    B - V: +1.22, +1.43.
UW    Mus    Min II 11.9.
UY    Mus    Min II 12.0.
VW    Mus    Min II 13.9.
WY    Mus    P var. Periodic term: +0.35d*sin(0.12deg*E).
XZ    Mus    Before JD2419200 Max = 2412590 + 113d*E.
AB    Mus    Min II 13.0.
AS    Mus    [A/H] = 0.5.
AX    Mus    P var. During JD2412550 - 19200 - see Table; during
AX    Mus    JD2423900 - 26100 P = 97.3d.
AY    Mus    Min II 10.8. Min II - Min I = 0.481P.
AY    Mus    The elements are valid during 1897 - 1943. In the time
AY    Mus    interval JD2441683 - 721 eclipses did not occur [08094].
BB    Mus    P, possibly P should be doubled.
BD    Mus    Depth of Min II 0.05m.
BE    Mus    Min II 14.1.
BF    Mus    Min II 14.4.
BK    Mus    P very long P: 56d < d < 310d.
BR    Mus    Min II 11.25. B - V: +0.10m.
BS    Mus    Min II 11.5.
BX    Mus    Depth of Min II 0.04m.
CD    Mus    Min II 14.7.
CS    Mus    P > 120d.
DW    Mus    According to [08135], the spectral type is M5e, typical of
DW    Mus    Mira stars. Elements in [03934] were deduced from the
DW    Mus    observed brightness variations with P ~355d which
DW    Mus    was considered to be a spurious period; rapid variations
DW    Mus    were confirmed by 7h of photographic observations.
DZ    Mus    Possibly Pshould be doubled.
EE    Mus    In the coal sack. The flare was observed spectroscopically.
EN    Mus    d = 0.035P:.
EP    Mus    [A/H] = 0.2. According to [08136], EA,
EP    Mus    P = 4.15d, D = 0.05P, 11.63m - 12.60m V, Min II 11.7:.
ET    Mus    Alternatively possible type EW [08727, 04001].
EV    Mus    d = 0.09P:.
EY    Mus    In the Coal Sack region.
EZ    Mus    Alternative possible values of P 4.3032d, 4.3224d.
FH    Mus    Depth of Min II 0.03m.
FO    Mus    P var?
GK    Mus    Min II 15.0.
GN    Mus    Min II 14.2.
GO    Mus    Min II 15.2.
GP    Mus    B - V: +1.03, +1.61.
KU    Mus    Type RV: is also possible.
MR    Mus    MinII 8.53.
NT    Mus    VB A (B 12.8m, 14", 233deg, 2000).
OT    Mus    VB, several companions within 15".
OW    Mus    A twice longer period is not excluded.
PX    Mus    The mean brightness varies with a possible period about 750d.
QR    Mus    VB A (B 14.3mpg, 18", 228deg, 2000).
QU    Mus    VB A (B 14.7mpg, 13", 183deg, 2000).
V0338 Mus    Min II = 10.1. VB AB (10.14m, 11.00m, 2.4", 129deg, 1985).
V0340 Mus    Min II = 8.06.
alf   Mus    VB A (B 13.0m, 29.3", 316deg).
eta   Mus    VB A (B 7.30m, 60").
tet   Mus    VB (A 5.64m, B 7.5m, 5.3", 187deg); SB (Porb = 18.341B).
tet   Mus    Variable intensity of emission lines with respect to the
tet   Mus    continuum (double wave; elements in the Table are for the
tet   Mus    epochs of Min I variability in the UV range (lambda lambda
tet   Mus    1550 - 3300 A) with an amplitude about 2%, P = 1.5d and
tet   Mus    rapid changes (lamda lamda 1550 - 1800 A) with an
tet   Mus    amplitude about 3 - 5% on the time scale of 50s - 70s
tet   Mus    [08532]. Connected with a nebula, 80'*45'.
R     Nor    VB A (B 14.0m, 5.7", 268deg, 1929). P var. Max II =
R     Nor    2406371 + 486.94d*E (JD2406300 - 25000); Max II =
R     Nor    2426359 + 500.56d*E (JD2426000 - 30500); Max II =
R     Nor    2431377 + 489.0d*E (JD2430500 - 34500); since
R     Nor    JD2437600 - see Table. Like R Cen, has a doudle Max,
R     Nor    JD2437600 - see Table. Like R Cen, has a doudle Max,
R     Nor    divided by a comparatively shallow Min II. Max II is
R     Nor    usually brighter than Max I. Phase (Min I) = 0.43P,
R     Nor    Phase (Max I) = 0.70P, Phase(Min II) = 0.85P.
S     Nor    In the centre of the open cluster NGC 6087, cluster member.
S     Nor    [A/H] = -0.1.
T     Nor    P var.Max = 2414783 + 241.87d*E (JD2414700 - 28000);
T     Nor    Max = 2428084 + 244.93d*E (JD2428000 - 35000);
T     Nor    since JD2437000 - see Table.
U     Nor    P var. Max = 2415028.94 + 12.64084d*E (JD2415000 - 26000)
U     Nor    [00060]; since JD2434000 - see Table, [A/H] = -0.6.
W     Nor    P2 ~1300d.
Y     Nor    VB A (B 12.2m vis, 4.0", 156deg, 1903).
Z     Nor    Min II 9.6.
RR    Nor    Min II 9.9.
RS    Nor    B - V: +1.13,  +1.48.
RT    Nor    Quasiperiodic variations: P1 ~59d, P2 ~175d [08140].
RV    Nor    [A/H] = 0.8.
RV    Nor    There are irregularities in the light curve.
SV    Nor    Min II 12.6.
SW    Nor    D = 0.013P, d = 0.003P.
SX    Nor    d = 0.1P.
SY    Nor    VB A (B 12.8m, 2.1", 315deg, 1934). B - V: +1.16,  +1.49.
SY    Nor    [A/H] = 0.5.
SZ    Nor    Min II 12.6.
TT    Nor    Twice longer P is possible.
TU    Nor    Min II 12.5. Associated with a small faint nebula.
TV    Nor    Min II 9.3.
TW    Nor    In the region of the poor open cluster Lynga 6.
TW    Nor    B - V: +1.79, +2.22. [A/H] = 0.2.
TX    Nor    Min II 12.5.
TZ    Nor    Min II 12.1.
UV    Nor    d ~0.07P.
UX    Nor    In Max light B - V = +0.30.
UY    Nor    d = 0.025P.
UZ    Nor    d = 0.02P.
VV    Nor    In the region of the cluster NGC 6152.
VX    Nor    Depth of Min II ~0.03m.
VZ    Nor    In the region of the cluster NGC 6152. Min II 14.3.
WX    Nor    The chart is erroneously labelled as that for WZ Nor.
WX    Nor    Min II 12.8.
WZ    Nor    The chart is erroneously labelled as that for WX Nor.
WZ    Nor    Min II 13.4.
XY    Nor    Min II 13.2.
AA    Nor    [A/H] = -0.1.
AF    Nor    In the region of the open cluster NGC 5999.
AQ    Nor    The chart in [06286] is wrong.
AR    Nor    The chart in [06286] is wrong.
AT    Nor    d = 0.026P:.
BE    Nor    Min II 14.2.
BF    Nor    The chart in [06286] is wrong.
BH    Nor    Min II 13.2.
BP    Nor    Close companion.
CE    Nor    d = 0.05P. Min II 11.8?
CG    Nor    The chart in [06286] is wrong.
CI    Nor    The chart in [06286] is wrong.
CT    Nor    The chart in [06286] is wrong.
CX    Nor    Min II 15.0.
DE    Nor    The chart in [06286] is wrong.
DF    Nor    The chart in [06286] is wrong.
DO    Nor    Min II 14.2. In the region of the open cluster NGC 6087.
DP    Nor    The chart in [06286] is wrong.
DR    Nor    In the region of the open cluster NGC 6087.
EE    Nor    The chart in [06286] is wrong.
EM    Nor    Min II 13.8.
ET    Nor    d = 0.032P.
FG    Nor    The chart in [06286] is wrong.
FI    Nor    The chart in [06286] is wrong.
FK    Nor    Min II 15.0.
FQ    Nor    According to [00060], P = 1.994d?
FW    Nor    Min II 14.5.
GM    Nor    d = 0.02P; Min II 11.01; Min II - Min I = 0.499P
GM    Nor    (JD2441683 - 721), Min II - Min I = 0.531P (JD2425381 -
GM    Nor    28402). B - V = 0.44m.
GN    Nor    Min II 13.3, DII = 0.16P, Min II - Min I = 0.405P
GN    Nor    (JD2425900). Apsidal motion: P = 500yr.
GO    Nor    Min II 13.7.
GQ    Nor    Min II 13.8.
GR    Nor    [A/H] = 0.9.
GT    Nor    d = 0.048P.
GU    Nor    In the region of the open cluster NGC 6067.
GU    Nor    B - V: +1.17, +1.40. [A/H] = 0.1.
GV    Nor    d = 0.03P:.
GX    Nor    Min II 15.0.
HH    Nor    VB B (A 9.9m vis, FO; B 12.6", 148deg). d = 0.05P.
HI    Nor    D is very small.
HK    Nor    Min II 12.9.
HO    Nor    Min II 13.2:.
HW    Nor    d = 0.024P.
HZ    Nor    P = 2.921584d is possible.
IQ    Nor    B - V: +1.55, +1.93.
IS    Nor    In the region of the open cluster NGC 6067.
IT    Nor    Min II 9.8.
KL    Nor    P >= 140d.
KM    Nor    P >= 170d.
KQ    Nor    Mira Ceti type is not excluded [04001].
KT    Nor    P >= 180d.
KX    Nor    Min II 14.8.
LO    Nor    P >= 220d.
LV    Nor    Deep Min II.
LX    Nor    Possible P values: 0.60492d, 0.7851d, etc.
NR    Nor    Min II 15.9.
NS    Nor    Min II 10.50 V; Min II - Min I = 0.67P
NW    Nor    P > 140d.
NX    Nor    Min II 14.4.
OS    Nor    Epoch of Min is given. EW/KW type is possible.
OT    Nor    Min II 13.7.
OU    Nor    Min II 15.1.
OV    Nor    P >= 200d.
OW    Nor    P >= 120d.
OX    Nor    P >= 110d.
PQ    Nor    Possibly a cepheid which is a fainter component of an
PQ    Nor    unresolved binary. Epoch of Max is given.
PT    Nor    In the region of the open cluster NGC 6067.
QT    Nor    HV 5388 = HV 8903. The coordinates in [00424] are wrong.
QV    Nor    3U 1538 - 52. No.12 [04124].
QV    Nor    Epoch of Min corresponding to the X-ray eclipse is given.
QV    Nor    Depth of Min I 0.05m V, that of Min II 0.08m V. The period
QV    Nor    of X-ray pulses Px = 528.928s [04114]. A flare was observed
QV    Nor    with Delta(m) > 0.3m [09456].
QX    Nor    4U 1608 - 52.
QZ    Nor    In the open cluster NGC 6067.
V0367 Nor    May be not a supergiant.
V0374 Nor    Type LBV: is also possible.
V0384 Nor    MinII 10.30.
V0389 Nor    Min II 15.7.
V0392 Nor    VB (A 8.59m; B 9.29m, 13", 205deg, 2000). The combined brightness is tabulated.
V0396 Nor    Cluster non-member. MinII - MinI = 0.44P.
V0405 Nor    Min II = 9.08:. MinII - MinI = 0.56P.
V0410 Nor    Min II = 16.60.
V0412 Nor    Min II = 16.90:. O'Connell effect.
V0413 Nor    Min II = 15.80.
V0414 Nor    Min II = 14.95:.
V0415 Nor    Min II = 17.90.
V0417 Nor    Min II = 16.65.
V0418 Nor    Min II = 16.45.
V0419 Nor    Min II = 16.35.
V0420 Nor    Min II = 17.95.
V0422 Nor    Min II = 17.50.
V0424 Nor    Min II = 14.73.
V0426 Nor    Min II = 18.0.
V0427 Nor    Min II = 16.78.
V0428 Nor    Min II = 13.22.
V0429 Nor    The coordinates in [419] are wrong.
V0430 Nor    Min II = 17.18. The coordinates in [419] are wrong.
V0432 Nor    Min II = 17.30.
V0434 Nor    Min II = 16.45.
V0436 Nor    Min II = 17.65.
V0437 Nor    Min II = 14.10.
V0438 Nor    Min II = 17.0.
V0440 Nor    Min II = 16.13.
V0441 Nor    Min II = 16.6.
V0442 Nor    Min II = 14.95.
V0443 Nor    Min II = 16.8.
V0445 Nor    Min II = 17.2.
V0447 Nor    Min II = 16.62.
V0448 Nor    Min II = 16.50.
V0449 Nor    Min II = 15.75.
V0451 Nor    Min II = 9.58.
V0479 Nor    Multiperiodic; P2 = 0.204945d.
mu.   Nor    In the region of the open cluster NGC 6169.
U     Oct    P var. Max = 2420685 + 302.00d*E (JD2414900 -
U     Oct    20700); Max = 2424320 + 300.74d*E (JD2422800 -
U     Oct    29800); Max = 2431901 + 309.60d*E (JD2429800 -
U     Oct    32250); Max = 2434018 + 300.70d*E (JD2432250 -
U     Oct    38800); since JD2438800 - see Table.
X     Oct    P var.Max = 2415170 + 208.40d*E (JD2415100 -
X     Oct    17100); Max = 2417425 + 201.24d*E (JD2417100 -
X     Oct    20700); Max = 2423780 + 207.95d*E (JD2422000 -
X     Oct    24000); Max = 2424370 + 200.18d*E (JD2424000 -
X     Oct    25600); since JD2425600 - see Table. Depths of minima are
X     Oct    stongly variable; 1.1m <= A <= 4.0m.
RV    Oct    Delta(S) = 10.
TX    Oct    Min II 12.7.
UV    Oct    Delta(S) = 9; (k - b)2 = 0.06. Blazhko effect: P = 80d;
UV    Oct    0.14P <= M - m <= 0.24P, 0.4m <= A <= 1.3m.
UZ    Oct    Min II 9.48; dI = 0.00P, dII = 0.05P. P var. Min I =
UZ    Oct    2440223.1560 + 1.1493709d*E (JD2438300 - 42000);
UZ    Oct    since JD2442000 - see Table.
AM    Oct    Min II 14.9.
BC    Oct    Min II 10.8:V. Also possible is P=26.45924 with MinII - MinI = 0.338P.
BE    Oct    P < 20d:.
BG    Oct    P = 0.7490d?
BK    Oct    Min II 14.6.
BP    Oct    (k - b)2 = 0.25.
CC    Oct    Basic radial pulsation with P1 = 0.12490d (A1 = 0.042m)
CC    Oct    is superimposed by others with periods: P2 = 0.0795317d
CC    Oct    (A2 = 0.008m), P3 = 0.12336d (A3 = 0.014m); P4 =
CC    Oct    0.11068d (A4 = 0.008m), P5 = 0.12713d (A5 = 0.006m);
CC    Oct    P6 = 0.11815d (A6 = 0.006m).
CD    Oct    mu = 0.51", p = 279deg. One of the periods P = 686s
CD    Oct    (A = 0.01m).
CE    Oct    Light oscillation with P2 = 0.054511d (A2 = 0.0056m) is
CE    Oct    superimposed by an oscillation with P1 = 0.2100d or
CE    Oct    0.2660d (A1 = 0.0052m), which is due to pulsation or
CE    Oct    ellipsoidal variability in a close binary system.
CP    Oct    Variability type and spectral type (F2/F3Ib/II) do not agree.
DU    Oct    MinII 9.34.
DV    Oct    In the constellation Octans.
DZ    Oct    Blazhko effect, P=36.8d.
EV    Oct    Min II = 14.5.
EX    Oct    Min II = 11.20.
EZ    Oct    Min II = 12.04.
alf   Oct    SB, Porb = 9.073d.
R     Oph    P var. Max = 2399214 + 302.1d*E (JD2399200 - 2427900)
R     Oph    [00458]; Max = 2427915 + 304.0d*E (JD2427900 - 34900);
R     Oph    Max = 2434906 + 301.5d*E (JD2434900 - 40600) [00001];
R     Oph    since JD2440600 - see Table.
U     Oph    ADS 10428 A (B 12.26m, GOV, 20.4", 358deg). Min II 6.46.
U     Oph    P var. Periodic term:
U     Oph    +0.0120d*sin(0.0483deg*E + 4.7833deg).
V     Oph    P var. Max = 2411155 + 296.73d*E (JD2411000 - 24000);
V     Oph    Max = 2424198 + 302.46d*E (JD2424000 - 28000);
V     Oph    since JD2428000 - see Table.
W     Oph    P var. Before JD2420500 Max = 2415186 +
W     Oph    335.07d*E; Max = 2420870 + 325.33d*E (JD2420500 -
W     Oph    24700); since JD2424700 - see Table.
X     Oph    VBA (A = 0.34", Porb = 485.3 yr; B - 9m, K1III, 0.4",
X     Oph    142deg, 1980).
X     Oph    The range of the combined brightness is given.
X     Oph    P var. Max = 2416416 + 336.61d*E (JD2416400 - 26000);
X     Oph    Max = 2426161 + 331.28d*E (JD2426000 - 32500); Max =
X     Oph    2432788 + 335.50d*E (JD2432500 - 38000);
X     Oph    since JD2438000 - see Table.
Y     Oph    SB1? Porb = 2612d? P var. Before JD2427000
Y     Oph    Max = 2408694.77 + 17.11884d*E; since
Y     Oph    JD2432000 - see Table. [A/H] = -0.2.
Z     Oph    P var. Max = 2411896 + 349.0d*E (JD2411800 - 21000)
Z     Oph    [00458]; Max = 2420962 + 352.1d*E (JD2421000 - 25000);
Z     Oph    Max = 2425183 + 347.4d*E (JD2425000 - 31000);
Z     Oph    Mean elements after JD2431000 - see Table.
RR    Oph    P var. Nonlinear term: -0.009282d*E2.
RS    Oph    Previous outbursts: 1898, 1933, 1958.
RS    Oph    According to [07575], in 1972 - 1973 there were semiregular
RS    Oph    variations (Delta(m) ~0.5M, P = 50D - 70D).
RT    Oph    P var. Before JD2426500 Max = 2417452 +
RT    Oph    429.00d*E; Max = 2426461 + 422.67d*E (JD2426500 -
RT    Oph    34000); since JD2434500 - see Table. OH, H2O maser.
RU    Oph    P var. Before JD2422000 Max = 2417388 +
RU    Oph    200.95d*E; Max = 2422011 + 203.62d*E (JD2422000 -
RU    Oph    27300); Max = 2427298 + 200.5d*E (JD2427300 - 29000);
RU    Oph    Max = 2429305 + 203.88d*E (JD2429000 - 33000);
RU    Oph    during JD2433000 - 40500 - see Table.
RV    Oph    d = 0.015P; Min II 9.56, DII = 0.09P. The light curve
RV    Oph    share var.
RW    Oph    P var. Max = 242494 + 247.86d*E (JD2425000 - 34000).
RW    Oph    The Table gives mean elements.
RX    Oph    OH, H2O maser.
RY    Oph    P var. Max = 2415235 + 151.05d*E (JD2414700 - 24000);
RY    Oph    Max = 2424152 + 149.69d*E (JD2424000 - 31000); Max =
RY    Oph    2431339 + 150.94d*E (JD2431000 - 40000);
RY    Oph    since JD2440000 - see Table.
RZ    Oph    d = 0.030P.
SS    Oph    P var. Before JD2432500 Max = 2417330 + 179.88d*E.
ST    Oph    (k - b)2 = 0.03.
SV    Oph    The elements are valid since JD2422000.
SW    Oph    VB A (B 12.0m vis, 2.4", 91deg, 1943). d = 0.02P. P var.
SW    Oph    Min = 2418880.528 + 2.445948d*E (JD2418880 - 26200)
SW    Oph    [00001]; Min = 2431235.216 + 2.446086d*E (JD2427900 -
SW    Oph    33500) [02389]; since JD2434000 - see Table.
SX    Oph    d = 0.03P.
SZ    Oph    P var. Before JD2428400 Min = 2421057.556 + 3.708454d*E;
SZ    Oph    since JD2442000 - see Table.
TT    Oph    [Fe/H] = -0.5.
TW    Oph    P2 = 2000d:. Associated with a nebula of variable
TW    Oph    brightness [03479].
UU    Oph    d = 0.024P. P var?
UX    Oph    P var. Max = 2426041 + 117.34d (JD2406430 - 28040);
UX    Oph    since JD2433100 - see Table.
VW    Oph    P var. Mean elements are given. During JD2422500 - 30600
VW    Oph    Max = 2430554 + 282.69d*E.
WW    Oph    Epoch of Min is given. The chart in [06286] is wrong.
WZ    Oph    Min II 9.82.
XX    Oph    A symbiotic object featuring deep fadings
XX    Oph    of long duration [09489].
AH    Oph    H2O maser.
AQ    Oph    The chart in [06286] is wrong.
BE    Oph    The data in [00278] refer to another star.
BF    Oph    SB? P var? since JD2430000 - see Table.
BN    Oph    80d <= P <= 250d.
DM    Oph    P var. P = 220d (1893 - 1910), P = 216d (1914 - 1928).
DQ    Oph    P = 35d is possible.
FK    Oph    V2 (NGC 6273).
GM    Oph    V12 (NGC 6284).
GR    Oph    P var. Max = 2415425 + 136d*E (1893 - 1908);
GR    Oph    during 1910 - 1928 - see Table.
IL    Oph    P2 = 140d:.
IW    Oph    In the field of the globular cluster NGC 6293,
IW    Oph    possible cluster member.
KM    Oph    In the field of the globular cluster NGC 6304, field star.
KO    Oph    In a dark nebula.
KQ    Oph    P2 = 1500d.
KR    Oph    P2 > 5000d.
OU    Oph    V70 (NGC 6266).
PU    Oph    VB (A = V29 (NGC 6266), the data are in the Table; B = V28
PU    Oph    (NGC 6266), 16.6m - 17m, 4B, 4.8", 7deg), B: RRAB,
PU    Oph    Max = 2433423.52 + 0.49749d*E, M - m = 0.15P.
V0378 Oph    Min II 14.2. In the region of the open cluster CR 359.
V0378 Oph    Epoch of Max is given.
V0380 Oph    Porb = 0.16d. Blue.
V0391 Oph    In the region of the open cluster CR 359. P var?
V0391 Oph    Before JD2427000 Min = 2425501.425 + 2.89558d*E [00432];
V0391 Oph    since JD2441500 - see Table.
V0392 Oph    Red.
V0402 Oph    P var. Max = 2425364 + 154d*E (JD2425350 - 670);
V0402 Oph    since JD2425670 - see Table.
V0413 Oph    Delta(S) = 3. Blazhko effect?
V0414 Oph    B - V: +0.41, +0.77.
V0423 Oph    In the region of the open cluster CR 359.
V0426 Oph    Outbursts separated by 17d - 55d [08079]; in 1976 - 77 the
V0426 Oph    cycle was 32.3d. Outside outbursts 12.7m - 13.3m, waves
V0426 Oph    with a cycle of 20 - 30 Min and slower variations.
V0438 Oph    H20 Maser.
V0439 Oph    B - V: +0.63, +0.97.
V0442 Oph    Porb = 0.14056d.
V0445 Oph    VB A (B 13.04m y, 21"nf). (k - b)2 = 0.35; Delta(S) = 2.
V0445 Oph    According to [05692], Blazhko effect (Pi > 2000d).
V0449 Oph    P var. Before JD243900 Min = 2428696.465 +
V0449 Oph    1.243078d*E; Min = 2442959.607 + 1.243095d*E
V0449 Oph    (JD2439000 - 43000); since JD2443000 - see Table.
V0451 Oph    Min II 8.31; Min II - Min I = 0.494P; DII = 0.12P.
V0452 Oph    Delta(S) = 5:.
V0455 Oph    P var? The Table gives mean elements which need
V0455 Oph    confirmation.
V0456 Oph    Min II 10.5. P var. Before JD2436100 Min =
V0456 Oph    2428422.341 + 1.015986d*E [00476]; since JD2441800 - see
V0456 Oph    Table.
V0465 Oph    B - V: +0.68, +1.10. P var?
V0471 Oph    Very red.
V0478 Oph    B - V: +0.86, +1.33. [A/H] = -0.7.
V0478 Oph    The elements need confirmation.
V0487 Oph    D <= 0.14P. In the region of the open cluster Cr 359.
V0496 Oph    In the region of the open cluster Cr 359.
V0501 Oph    Min II 11.1.
V0502 Oph    Min II 8.81. P var. Since JD2434500 - see Table.
V0506 Oph    Min II 12.0. In the region of the open cluster Cr 359.
V0508 Oph    Min II 10.59.
V0509 Oph    In the region of the open cluster Cr 359.
V0511 Oph    Min II 13.7. In the region of the open cluster Cr 359.
V0515 Oph    Max = 2425600 + 300d*E (JD2425600 - 26700); P = 140d
V0515 Oph    (JD2426700 - 27300); during JD2427300 - 30200 - see Table.
V0516 Oph    In the region of the globular cluster NGC 6304.
V0517 Oph    In the region of the globular cluster NGC 6304.
V0521 Oph    P = 164d (JD2415000 - 24600); P2 - 4000d.
V0526 Oph    Min II 13.6.
V0527 Oph    Min II 14.8.
V0532 Oph    P >= 6000d.
V0533 Oph    P >= 80d.
V0534 Oph    d = 0.03P.
V0535 Oph    d = 0.025P.
V0536 Oph    d = 0.04P:.
V0537 Oph    Min II 12.8.
V0540 Oph    d = 0.05P; Min II 13.4.
V0541 Oph    [A/H] = -1.0. In the region of the globular cluster
V0541 Oph    NGC 6401; cluster non-member?
V0543 Oph    Min II 13.6.
V0549 Oph    Min II 14.0.
V0550 Oph    Min II 13.0.
V0554 Oph    [A/H] = -1.1.
V0555 Oph    Sharp and flat maxima. Blazhko effect?
V0557 Oph    Min II 15.7. In the region of the open cluster Cr 359.
V0558 Oph    B - V: +0.57, +0.68. [Fe/H] = -1.48. According to [09037],
V0558 Oph    P = 0.299d.
V0564 Oph    [Fe/H] = -1.37. Epoch of Min is given. P var. Nonlinear
V0564 Oph    term: +0.0073d*(E + 10)**2.
V0565 Oph    P = 0.3957d is possible. Photoelectric observations of
V0565 Oph    1968 contradict the elements [05746].
V0566 Oph    dI = 0.048P; Min II 7.89, dII = 0.06P. P var. Before
V0566 Oph    JD2440500 Min = 2436744.4200 + 0.40964091d*E [08287]; since
V0566 Oph    JD2440500 - see Table.
V0567 Oph    (k - b)2 = 0.22; Delta(S) = 0. According to [07984],
V0567 Oph    Max = 2441134.467 + 0.1300729d*E.
V0568 Oph    Red.
V0570 Oph    VB A (B 16.3m, 5", 90deg).
V0572 Oph    In the region of the open cluster Cr 359.
V0573 Oph    d = 0.034P. In the region of the open cluster Cr 359.
V0574 Oph    P2 ~500d.
V0577 Oph    Min II 11.9. Min II - Min I = 0.583P. DII = 0.050P.
V0577 Oph    e = 0.22.
V0580 Oph    VB A (B 15.5m, 0.2').
V0585 Oph    A long-period variation is superimposed?
V0586 Oph    In the region of the open cluster Cr 359.
V0590 Oph    Min II 13.6.
V0592 Oph    Max = 2427227 + 78d*E (JD2426100 - 29400);
V0592 Oph    during JD2429400 - 30150 - see Table.
V0592 Oph    After intervals of irregular variability the periodicity
V0592 Oph    resumes without phase shift.
V0605 Oph    Epoch of Min is given.
V0618 Oph    Min II 14.7:.
V0636 Oph    d = 0.030P.
V0683 Oph    P var. The light curve shape varies.
V0687 Oph    P may be twice longer.
V0693 Oph    Blazhko effect? [05692].
V0695 Oph    P var? The light curve shape varies.
V0698 Oph    P var? since JD2442950 - see Table.
V0700 Oph    B - V: +0.49, +0.50. [Fe/H] = -2.10.
V0716 Oph    Delta(S) = 7.
V0720 Oph    VI (NGC 6171). Cluster non-member.
V0722 Oph    P var. Max = 2437089.456 + 0.6190385d (JD2419900 - 37100)
V0722 Oph    [07806]; since JD2436700 - see Table.
V0729 Oph    P var. Max = 2437492.766 + 0.4685794d*E (JD2423500 - 37800)
V0729 Oph    [03560]; since JD2437400 - see Table.
V0732 Oph    Unusual light curve (sharp Max; primary Min; broad Max;
V0732 Oph    secondary Min 15.2).
V0734 Oph    P var. Max = 2420636.497 + 0.562489d*E (JD2420600 -
V0734 Oph    29100); during JD2429100 - 37150 - see Table.
V0735 Oph    Min II 10.6.
V0737 Oph    P = 374d is possible.
V0767 Oph    According to [00104], waves with Delta(m) = 0.3m - 1.4m vis
V0767 Oph    of 50d - 110d duration; mean brightness var,
V0767 Oph    Delta(m) ~0.4m in 800d - 1000d.
V0782 Oph    Very red.
V0784 Oph    B - V: +0.26, +0.56. The period should be checked.
V0786 Oph    Red.
V0788 Oph    Blazhko effect? Pi = 115d.
V0799 Oph    P = 215d is possible.
V0802 Oph    Red.
V0816 Oph    B - V: +0.25, +0.63.
V0822 Oph    Blazhko effect?
V0823 Oph    In the region of the open cluster IC 4665.
V0825 Oph    In the region of the open cluster IC 4665.
V0829 Oph    Blazhko effect? Pi = 165d.
V0832 Oph    Red.
V0838 Oph    P2 ~500d is possible.
V0839 Oph    mu = 0.041", ro = 292deg. Min II 9.38.
V0840 Oph    VB A (B 12m, 16", 116deg).
V0841 Oph    Max = 2396146.
V0843 Oph    SN Kepler. Max 2307193. Gaseous remnant.
V0844 Oph    Min II 14.9.
V0845 Oph    VB A (B 15.7m).
V0847 Oph    Min II 13.1.
V0848 Oph    Min II 13.4.
V0851 Oph    Max = 2425828 + 95d*E (JD2425600 - 29700);
V0851 Oph    during JD2429700 - 34250 - see Table.
V0854 Oph    According to [08116], the spectrum
V0854 Oph    resembles that of a T Tau - type star.
V0868 Oph    Min II 13.6. In the region of the open cluster Cr 359.
V0870 Oph    In the region of the open cluster Cr 359.
V0872 Oph    P = 0.825d is possible.
V0878 Oph    Min II 16.5. In the region of the open cluster Cr 359.
V0911 Oph    P2 = 81d, P3 = 114d. P4 > P3? Standstills up to 100d.
V0919 Oph    VB A (B sp).
V0920 Oph    Min II 15.9.
V0924 Oph    Min II 16.4.
V0929 Oph    d = 0.050P.
V0934 Oph    E type is possible.
V0936 Oph    In the region of the open cluster Cr 359.
V0938 Oph    Min II 15.3. In the region of the open cluster Cr 359.
V0940 Oph    Min II 15.6.
V0941 Oph    Min II 16.5.
V0943 Oph    Min II 16.4. In the region of the open cluster Cr 359.
V0945 Oph    Min II 15.1. In the region of the open cluster Cr 359.
V0947 Oph    Min II 14.5. In the region of the open cluster Cr 359.
V0952 Oph    P = 0.954d is possible.
V0954 Oph    In the region of the open cluster Cr 359. Min II 14.9.
V0954 Oph    According to [03500], const, V = 12.86m, B - V = +1.36m,
V0959 Oph    P var? Max = 2429785.419 + 0.084857d*E
V0959 Oph    (JD2429785 - 845) [02757]; during JD2443719 - 732 - see
V0959 Oph    Table; other possible elemente:
V0959 Oph    Max = 2443726.469 + 0.07786d*E.
V0960 Oph    In the region of the open cluster Cr 359.
V0963 Oph    Min II 15.1. In the region of the open cluster Cr 359.
V0968 Oph    [Fe/H] = -1.48. In the region of the open cluster Cr 359.
V0969 Oph    Min II 13.8:. In the region of the open cluster Cr 359.
V0977 Oph    In the region of the globular cluster NGC 6426.
V0978 Oph    In the region of the globular cluster NGC 6426.
V0979 Oph    V11 (NGC 6426). Cluster non-member.
V0980 Oph    In the the region of globular cluster NGC 6426.
V0980 Oph    P = 0.25740d is possible.
V0983 Oph    In the region of the open cluster Cr 359.
V0986 Oph    In July 1980 Vr varied with P = 0.179d, 0.147d, 0.225d,
V0986 Oph    and possibly 0.097d, but there were no spectrum variations,
V0986 Oph    and the photometric P = 0.323d was not noticeable in Vr.
V0986 Oph    SB? Porb = 15d - 20d; there is also excess power
V0986 Oph    at low frequences in the photometric data. Earlier
V0986 Oph    studies revealed photometric periods 0.284d - 0.4d
V0986 Oph    and violation of periodicity.
V0987 Oph    d = 0.02P. Min II 14.6. In the region of the open cluster
V0987 Oph    Cr 359.
V0998 Oph    In the region of the globular cluster NGC 6171.
V0999 Oph    In the region of the globular cluster NGC 6171.
V1000 Oph    Blazhko effect?
V1002 Oph    Min II 15.2.
V1002 Oph    RRC type with twice shorter P is possible.
V1004 Oph    Blazhko effect?
V1010 Oph    Min II 6.46. P var. P = 0.661464d (JD2415000 - 25000)
V1010 Oph    [05738]; since JD2425000 - see Table, nonlinear term:
V1010 Oph    -3.87d*10**(-10)*E**2. Min I var.The light curve shape and
V1010 Oph    the depth of Min I var.
V1011 Oph    Blazhko effect?
V1015 Oph    D <= 0.23P, d < 0.02P; Min II 14.5.
V1017 Oph    [Fe/H] = -1.25. P var? Max = 2437433.935 + 0.2343d*E
V1017 Oph    (JD2437433 - 514) [03625]. During
V1017 Oph    JD2442954 - 45140 - see Table.
V1017 Oph    According to [09037], P = 0.361d.
V1018 Oph    Possibly eclipsing.
V1021 Oph    Delta(m) var. B - V: +0.42, +0.62.
V1022 Oph    d = 0.06P:; Min II 15.95.
V1024 Oph    Max = 2437433.559 + 0.5914d*E (JD2437433 - 514)
V1024 Oph    [03625]. During JD2442954 - 45140 - see Table.
V1024 Oph    RR(B) type is possible; P = 0.371d satisfies the
V1024 Oph    observations during JD2442954 - 44407.
V1026 Oph    Max = 2437433.562 + 0.6563d*E (JD2437433 - 514)
V1026 Oph    [03625]. During JD2442954 - 45140 - see Table.
V1028 Oph    Blazhko effect?
V1032 Oph    P > 1.0d is not excluded.
V1033 Oph    Max = 2437433.714 + 0.4845d*E (JD2437433 - 514)
V1033 Oph    [03625]. During JD2442954 - 45140 - see Table.
V1035 Oph    Max = 2437433.388 + 0.6100d*E (JD2437433 - 514)
V1035 Oph    [03625]; during JD2442954 - 45140 - see Table.
V1039 Oph    P = 0.3166d is possible.
V1040 Oph    The light curve shape var.
V1041 Oph    [Fe/H] = -1.06.
V1042 Oph    The light curve shape var. Max = 2437433.633 + 0.5528d
V1042 Oph    (JD2437433 - 514) [03625]. During JD2442954 - 45140 - see
V1042 Oph    Table.
V1052 Oph    Max = 2437433.537 + 0.7546d*E (JD2437433 - 514)
V1052 Oph    [03625]; during JD2442954 - 45140 - see Table.
V1054 Oph    VB Wolf 630AB (A 9.76m V, 12.47mu; B 9.78m V; A = 0.22",
V1054 Oph    Porb = 1.71665 yr; C = Wolf 629, 11.70m V,14.75mu,
V1054 Oph    dM4, 72", D = vB8, 16.7m V, 221", common mu). mu = 1.19",
V1054 Oph    ro = 222deg. Lx/Lopt(V) = 0.05.
V1072 Oph    P var. Max = 2439025.31 + 0.444715d*E (JD2438500 - 39025);
V1072 Oph    since JD2442800 - see Table.
V1075 Oph    Red.
V1077 Oph    P var. Max = 2438614.40 + 0.373926d*E (JD2438200 - 700);
V1077 Oph    Max = 2442871.516 + 0.37384d*E (JD2442810 - 910):
V1077 Oph    Max = 2442983.345 + 0.373911d*E (JD2442920 - 3330);
V1077 Oph    since JD2443330 - see Table.
V1089 Oph    VB AB (B 16.4m, 2", 45deg).
V1099 Oph    Red.
V1100 Oph    Red.
V1111 Oph    OH, H2O, SiO maser.
V1120 Oph    Min II 14.3.
V1121 Oph    Soft X-ray source.
V1135 Oph    [Ca/H] = -0.74.
V1141 Oph    P var? The light curve shape var?
V1142 Oph    P var? The light curve shape var?
V1146 Oph    P = 185.2d is possible.
V1153 Oph    P = 153.0d is possible.
V1157 Oph    B - V: +0.42, +0.66.
V1161 Oph    P = 0.49d is possible [06438].
V1168 Oph    P var? The light curve shape var?
V1170 Oph    P = 360d: is possible [06438].
V1174 Oph    P var? The light curve shape var?
V1176 Oph    P = 269.0d is possible.
V1179 Oph    P var? The light curve shape var?
V1185 Oph    Other possible elements: Max = 2435630 + 177d*E [00001].
V1195 Oph    One more Max 2435637 (1956). Type M is possible.
V1203 Oph    P = 315d is possible [06438].
V1204 Oph    P = 144d: or P = 191d: are possible.
V1235 Oph    UV type is possible.
V1240 Oph    P = 0.42136d is possible.
V1244 Oph    The light curve shape var?
V1258 Oph    P var?
V1261 Oph    The light curve is not typical for the P in the Table [06438].
V1262 Oph    The light curve is not typical for the P in the Table [06438].
V1276 Oph    [Ca/H] = -0.1.
V1296 Oph    [Ca/H] = -0.9.
V1299 Oph    The light curve shape var?
V1300 Oph    P = 235d: is possible.
V1305 Oph    Min II 17.9:.
V1307 Oph    The light curve shape var? Spurious period? [06438].
V1323 Oph    P var?
V1332 Oph    [Ca/H] = -0.64.
V1348 Oph    The light curve shape var?
V1355 Oph    The light curve shape var?
V1403 Oph    P = 215d?
V1423 Oph    The light curve shape var?
V1426 Oph    P var?
V1451 Oph    P = 179.4d?
V1474 Oph    P = 127d:?
V1491 Oph    P = 328.0d?
V1492 Oph    The light curve shape var?
V1505 Oph    P = 86d:?
V1512 Oph    The light curve shape var?
V1526 Oph    P = 0.29745d?
V1532 Oph    P = 144.4d?
V1534 Oph    P = 198.8d?
V1548 Oph    The minor planet (336) Lacadiera.
V1554 Oph    P = 136.0d?
V1568 Oph    P = 275.5d?
V1571 Oph    P var?
V1573 Oph    Type E?
V1583 Oph    P - spurious?
V1616 Oph    Type E?
V1628 Oph    The light curve shape var?
V1637 Oph    [Ca/H] = -0.44.
V1661 Oph    The light curve shape var?
V1666 Oph    P = 154.2d?
V1676 Oph    Close optical companion?
V1682 Oph    P = 118.0d?
V1687 Oph    Type CW?
V1702 Oph    P = 121d?
V1705 Oph    P var?
V1710 Oph    P = 0.37422d?
V1731 Oph    The light curve shape var?
V1736 Oph    P = 143.8d?, P = 244.5d?
V1744 Oph    P = 191.6d?
V1748 Oph    A var. Type CW?
V1754 Oph    P = 128.4d?
V1768 Oph    The light curve shape var?
V1775 Oph    Type EW?
V1793 Oph    P = 170d:?
V1803 Oph    The star is not SVS 438.
V1805 Oph    The light curve shape var?
V1811 Oph    Min II 17.9:.
V1814 Oph    P = 160.4d?
V1822 Oph    P var?
V1829 Oph    P = 143.2d?
V1840 Oph    V 12 (NGC 6333 = M9). Cluster member.
V1841 Oph    The light curve shape var?
V1845 Oph    V7 (NGC 6333 = M9). Cluster member.
V1853 Oph    The light curve shape var?
V1860 Oph    [Ca/H] = -0.49.
V1861 Oph    P = 142.0d?
V1864 Oph    V3 (NGC 6333 = M9). Cluster member.
V1886 Oph    The light curve shape var?
V1889 Oph    P = 316.0d?
V1895 Oph    The light curve shape var?
V1905 Oph    P = 149.0d?
V1919 Oph    P = 102.8d?, P = 227.0d?
V1939 Oph    P = 330.0d?
V1946 Oph    The light curve shape var?
V1952 Oph    P = 248.0d?
V1953 Oph    P = 199d:?, P = 235d:?
V1954 Oph    P = 159.6d?
V1973 Oph    P = 0.24154d?
V1989 Oph    A var?
V1990 Oph    P = 121d:?
V1991 Oph    The light curve shape var?
V1994 Oph    P = 170.0d?
V1998 Oph    P = 270.5d?
V2002 Oph    The light curve shape var?
V2003 Oph    [Ca/H] = -0.96.
V2009 Oph    V5 (NGC 6356). Cluster member.
V2010 Oph    [CA/H] = -0.79.
V2016 Oph    [CA/H] = -0.96.
V2042 Oph    P var. Max = 2430146.478 + 0.5385d*E (JD2429100 -
V2042 Oph    30202); since JD2436700 - see Table.
V2045 Oph    The chart in [05159] is wrong.
V2048 Oph    SB2 [06598]. In the region of the open cluster Cr 359.
V2048 Oph    Along with irregular light variations typical for be stars
V2048 Oph    there are rapid flares with the amplitudes up to 1.8m
V2048 Oph    (lambda eff = 5800 A) [06150]. It is not excluded that the
V2048 Oph    flares occur on a fainter companion of the system.
V2051 Oph    Usually - 15.0m with strong flickering of brightness
V2051 Oph    (up to 0.4m is 5 minutes) and rare flares. At the same
V2051 Oph    time the eclipses are observed with depth to 2.5m with the
V2051 Oph    elements: Min = 2444787.32124 + 0.062427865d*E [09550];
V2051 Oph    D = 0.0088P:, d = 0.0065P.
V2058 Oph    In the dark nebula in the rho Oph region.
V2059 Oph    In the dark nebula in the rho Oph region.
V2061 Oph    In the region of the globular cluster NGC 6171 (M 107).
V2062 Oph    In the dark nebula in the rho Oph region.
V2063 Oph    The minor planet (64) Angelina.
V2064 Oph    In the dark nebula in the rho Oph region.
V2101 Oph    In a dark nebula.
V2102 Oph    In the region of the globular cluster NGC 6293.
V2105 Oph    Vr = 100 km/s.
V2106 Oph    Vr = -102 km/s.
V2108 Oph    H2O, SiO maser.
V2112 Oph    The primary oscillation with A1 = 0.0172m
V2112 Oph    (see Table) is superimposed by the secondary one
V2112 Oph    (A2 = 0.0061m) with the elements:
V2112 Oph    Max = 2444114.531: + 0.1449461d*E.
V2116 Oph    X-ray pulsar. The pulse period is decreasing: 135s (1971),
V2116 Oph    112.076s (1979), 109.668s (1980) [09553]. The spin-period
V2116 Oph    may be twice longer.
V2118 Oph    Probably rapidly rotating single spotted F type star.
V2118 Oph    Max brightness epoch is given.
V2119 Oph    In the region of the globular cluster
V2119 Oph    NGC 6284. Not a member of the cluster.
V2120 Oph    V6 (NGC 6284). In the region of the globular cluster
V2120 Oph    NGC 6284. Not a member of the cluster.
V2121 Oph    V10 (NGC 6284). In the region of the globular cluster
V2121 Oph    NGC 6284. Not a member of the cluster.
V2122 Oph    In the region of the globular cluster NGC 6284. Not
V2122 Oph    a member of the cluster.
V2123 Oph    V11 (NGC 6284). In the region of the globular cluster
V2123 Oph    NGC 6284. Not a member of the cluster.
V2124 Oph    In the region of the globular cluster NGC 6284. Not
V2124 Oph    a member of the cluster.
V2137 Oph    VB B (AB 3", 295deg).
V2391 Oph    Porb = 88.13yr. Component B is a suspected variable star
V2391 Oph    (NSV 24260) and may be the cause of variations.
V2561 Oph    Not a supernova.
V2577 Oph    The results in [246] do not refer to BE Oph [236].
V2597 Oph    P var.
V2600 Oph    MinII 12.6. Type EB according to [011].
V2604 Oph    MinII 14.0:.
V2609 Oph    P var.
V2612 Oph    MinII 9.70.
V2617 Oph    VB A (B 14.7mpg, 23", 166deg, 1999). The tabulated amplitude can be influenced by the companion.
V2626 Oph    MinII - MinI = 0.44P. VB (8.6mHp, 10.1mHp, 1.4", 306deg, 1991).
V2628 Oph    Period varies, the tabulated elements are valid for JD 2453000 - 2454600.
V2629 Oph    VB A (B 17.0mV, 13", 95deg, 2000).
V2636 Oph    A twice shorter period is not excluded.
V2638 Oph    A twice shorter period is not excluded.
V2640 Oph    VB A (B 13.8m, 25", 168deg, 2000).
V2642 Oph    A twice longer period is not excluded.
V2664 Oph    Period varies, current elements are tabulated.
V2666 Oph    VB AB (6.1mV, 7.0mV, 0.44", 308deg, 1992; a=1.19", Porb=294 years).
V2683 Oph    Blazhko effect, P = 26.28d [377].
V2690 Oph    Porb = 0.063791d.
V2703 Oph    VB A (B 14.3m, 19", 27deg, 1997).
V2709 Oph    Blazhko effect, P = 22.18d.
V2711 Oph    Multiperiodic.
V2715 Oph    VB, a close companion to the north-west.
V2718 Oph    Cluster non-member.
V2719 Oph    Cluster non-member. Type RRC a twice shorter period is not excluded.
V2720 Oph    Cluster non-member. Type EW with P=0.4225d is also possible.
V2721 Oph    Cluster non-member.
V2724 Oph    O'Connell effect.
V2731 Oph    Intermediate polar. Variations with Porb (see Table) and Pspin = 0.0014815d.
V2742 Oph    Biperiodic, P2 = 0.84443d.
V2744 Oph    The identification with NSV 09496 suggested in [80002] is wrong.
V2770 Oph    A one-day alias, P = 0.10096d, is also possible.
V2775 Oph    O'Connell effect.
V2780 Oph    The light curve shape varies.
V2787 Oph    O'Connell effect.
V2817 Oph    VB B (A 12.4m; AB 10", 34deg, 2000).
tet   Oph    SB1 (Porb = 11.44d [06597]).
tet   Oph    The basic oscillation (see Table) is superimposed by
tet   Oph    oscillations with the periods: P1 = 0.092551d,
tet   Oph    P2 = 0.069452d, P3 = 0.0555d, P4 = 0.0464d, P02 =
tet   Oph    0.137255d, P13 = 0.13845d, P24 = 0.13990d, P03 = 0.09185d.
khi   Oph    SB 1 (Porb = 138.8d [09558]).
ome   Oph    P = 1.5d?
R     Ori    SC 5/9.5 E. P var. Max = 2399420 + 378d*E
R     Ori    (JD2395600 - 99500); Max = 2412687 + 378.1d*E
R     Ori    (JD2403200 - 12700); Max = 2414230 + 366.5d*E
R     Ori    (JD2413800 - 16800); Max = 2417943 + 378.1d*E
R     Ori    (JD2416800 - 21350); Max = 2421352 + 384.9d*E
R     Ori    (JD2421350 - 24100); since JD2424100 - see Table.
S     Ori    VB A (B 10.9m, 47", 228deg). SiO maser. P var.
S     Ori    Max = 2404538 + 412.00d*E (JD2404520 - 13600);
S     Ori    Max = 2414014 + 427.15d*E (JD2414000 - 19150);
S     Ori    Max = 2419567 + 416.11d*E (JD2419570 - 22890);
S     Ori    Max = 2423312 + 407.10d*E (JD2423320 - 31050);
S     Ori    Max = 2431454 + 438.53d*E (JD2431500 - 39000)
S     Ori    [03765]; since JD2439000 - see Table.
T     Ori    In the T-association of the Orion nebula. Connected with
T     Ori    a cometary nebula.
U     Ori    SiO, OH, H2O maser. P var. Max = 2409881 + 374.5d*E
U     Ori    (JD2409800 - 15900); Max = 2415871 + 367.9d*E
U     Ori    (JD2415900 - 21000); Max = 2421016 + 376.0d*E
U     Ori    (JD2421000 - 29300); Max = 2428164 + 368.3d*E
U     Ori    (JD2428100 - 32900) [00960];
U     Ori    Max = 2433336 + 372.7d*E (JD2432900 - 43800);
U     Ori    since JD2443800 - see Table.
V     Ori    P var. Max = 2413656 + 264.8d*E (JD2411800 - 18700);
V     Ori    Max = 2418987 + 271.7d*E (JD2418700 - 24600);
V     Ori    Max = 2424695 + 263.7d*E (JD2424600 - 29400)
V     Ori    [00960]; Max = 2430769 + 269.9d*E (JD2430700 - 36200);
V     Ori    since JD2437700 - see Table.
W     Ori    Mean magnitude varies with P = 2450d.
Z     Ori    Min II 9.9; d = 0.013P.
RS    Ori    P var. Max = 2428073.205 + 7.566836d*E (JD2416500 -
RS    Ori    33000); since JD2435000 - see Table.
RT    Ori    Mean magnitude varies with P = 3200d.
RU    Ori    In the region of the nebula IC 434.
RV    Ori    In the region of the nebula IC 434.
RW    Ori    In the region of the nebula IC 434.
RX    Ori    In the region of the Orion nebula T-association.
RZ    Ori    In the region of the Orion nebula T-association.
SS    Ori    In the region of the Orion nebula T-association.
ST    Ori    In the region of the Orion nebula T-association.
SU    Ori    In the region of the Orion nebula T-association.
SV    Ori    In the region of the Orion nebula T-association.
SW    Ori    In the region of the Orion nebula T-association.
SX    Ori    In the region of the Orion nebula T-association.
SY    Ori    In the region of the Orion nebula T-association.
SZ    Ori    In the region of the Orion nebula T-association.
TT    Ori    In the region of the Orion nebula T-association.
TU    Ori    In the region of the Orion nebula T-association.
TV    Ori    In the region of the Orion nebula T-association.
TW    Ori    In the region of the Orion nebula T-association.
TX    Ori    VB A (B = TY Ori, 42.4", 45deg); in the region of
TX    Ori    the nebula IC 434.
TY    Ori    VB B (A = TX Ori); in the region of the nebula IC 434.
TZ    Ori    In the region of the nebula IC 434.
UW    Ori    Min II 11.6.
UY    Ori    In the region of the Orion nebula T-association.
UZ    Ori    In the region of the Orion nebula T-association.
VV    Ori    Min II 5.50; dI = 0.055P; dII = 0.064P.
VV    Ori    There is third component in the system
VV    Ori    (Porb = 119.09d [08045]).
VW    Ori    In the region of the Orion nebula T-association.
VX    Ori    In the region of the Orion nebula T-association.
VY    Ori    VB A (B = 16.6mV, 16", 135deg). In the region of the Orion
VY    Ori    nebula T-association.
VZ    Ori    In the region of the Orion nebula T-association.
WW    Ori    In the region of the Orion nebula T-association.
WX    Ori    VB A (B 17m, 11", 10deg). In the region of the Orion nebula
WX    Ori    T-association.
WY    Ori    In the region of the Orion nebula T-association.
WZ    Ori    In the region of the Orion nebula T-association.
XX    Ori    In the region of the Orion nebula T-association.
XY    Ori    In the region of the Orion nebula T-association.
XZ    Ori    The periodicity in light variations is possible.
XZ    Ori    In the region of the Orion nebula T-association.
YY    Ori    Emission. In the region of the Orion nebula T-association.
YZ    Ori    In the region of the Orion nebula T-association.
ZZ    Ori    In the region of the Orion nebula T-association.
AA    Ori    In the region of the Orion nebula T-association.
AB    Ori    In the region of the Orion nebula T-association.
AC    Ori    In the region of the Orion nebula T-association.
AE    Ori    In the region of the Orion nebula T-association.
AF    Ori    In the region of the Orion nebula T-association.
AG    Ori    VB A (B 16.4mV, 16", 185deg). In the region of the Orion
AG    Ori    nebula T-association.
AH    Ori    In the region of the Orion nebula T-association.
AI    Ori    In the region of the Orion nebula T-association.
AK    Ori    In the region of the Orion nebula T-association.
AL    Ori    In the region of the Orion nebula T-association.
AM    Ori    VB A (B 20.3mV, 3.5", 320deg). In the region of the Orion
AM    Ori    nebula T-association.
AN    Ori    In the region of the Orion nebula T-association.
AO    Ori    In the region of the Orion nebula T-association.
AP    Ori    In the region of the Orion nebula T-association.
AQ    Ori    In the region of the Orion nebula T-association.
AR    Ori    VB A (B 2", 240deg). In the region of the Orion nebula
AR    Ori    T-association.
AS    Ori    In the region of the Orion nebula T-association.
AT    Ori    In the region of the Orion nebula T-association.
AU    Ori    In the region of the Orion nebula T-association.
AV    Ori    VB A (B 18.7mV, 6", 305deg). In the region of the nebula
AV    Ori    T-association.
AW    Ori    In the region of the Orion nebula T-association.
AX    Ori    In the region of the Orion nebula T-association.
AY    Ori    In the region of the Orion nebula T-association.
AZ    Ori    In the region of the Orion nebula T-association.
BB    Ori    In the region of the Orion nebula T-association.
BC    Ori    In the region of the Orion nebula T-association.
BD    Ori    In the region of the Orion nebula T-association.
BE    Ori    In the region of the Orion nebula T-association.
BF    Ori    In the region of the Orion nebula T-association.
BG    Ori    In the region of the nebula IC 434.
BH    Ori    In the region of the Orion nebula T-association.
BK    Ori    P var. Max = 2422016 + 338.0d*E (JD2413550 - 22100);
BK    Ori    Max = 2428880 + 326.5d*E (JD2422300 - 28880);
BK    Ori    Max = 2429940 + 345.3d*E (JD2428880 - 29940);
BK    Ori    Max = 2432892 + 327.7d*E (JD2429940 - 32900);
BK    Ori    Max = 2438800 + 346.3d*E (JD2432900 - 38800);
BK    Ori    since JD2438800 - see Table.
BM    Ori    In the region of the Orion nebula T-association. In the
BM    Ori    cluster NGC 1976. Orion Trapezium
BM    Ori    member: teta**1 Ori B (A = V1016 Ori; B 8.7", 32deg;
BM    Ori    C 5.13m, 13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.05P;
BM    Ori    Min II 7.98. Shape of the light curve and depths of minima
BM    Ori    vary.
BO    Ori    In the region of the Orion nebula T-association.
BP    Ori    In the region of the Orion nebula T-association.
BS    Ori    In the region of the Orion nebula T-association.
BT    Ori    In the region of the Orion nebula T-association.
BU    Ori    In the region of the Orion nebula T-association.
BV    Ori    In the region of the Orion nebula T-association.
BW    Ori    In the region of the Orion nebula T-association.
BX    Ori    In the region of the Orion nebula T-association.
BY    Ori    In the region of the Orion nebula T-association.
BZ    Ori    In the region of the Orion nebula T-association.
CC    Ori    In the region of the Orion nebula T-association.
CD    Ori    In the region of the Orion nebula T-association.
CE    Ori    In the region of the Orion nebula T-association.
CF    Ori    In the region of the Orion nebula T-association.
CG    Ori    In the region of the Orion nebula T-association.
CH    Ori    In the region of the Orion nebula T-association.
CI    Ori    VB A (B 9.70m, 12.9", 88deg).
CM    Ori    P var?
CN    Ori    Porb = 0.163097d.
CN    Ori    Light curve is superposed by oscillations with
CN    Ori    the following elements: Max0 = 2444941.5032 +
CN    Ori    0.163097d*E (A0 = 0.2m), Max1 = 2444941.573 +
CN    Ori    0.15946d*E (A1 = 0.1m) [09471].
CN    Ori    Sometimes smaller rapid light oscillations are also
CN    Ori    observed with periods 24.3s - 29.5s (A<1%).
CO    Ori    Member of the T-association
CO    Ori    CO Ori. VB A (B 13m, 1", 280deg).
CP    Ori    Min II 11.2. P var [02545].
CT    Ori    SRD? P = 68d? [09496].
CW    Ori    Min II 13.2.
DK    Ori    In the region of the Orion nebula T-association.
DK    Ori    VB (ro < 3").
DL    Ori    In the region of the Orion nebula T-association.
DM    Ori    In the region of the Orion nebula T-association.
DN    Ori    Min II 9.9; d = 0.026P. P var. Min I = 2428497.51 +
DN    Ori    12.9649d*E (JD2425200 - 28600); since
DN    Ori    JD2435570 - see Table.
DY    Ori    B - V: +0.58, +1.72.
EG    Ori    d = 0.086P. P var?
EQ    Ori    Min II 10.3. P var. Min I = 2425889.706 + 1.74608d*E
EQ    Ori    (JD2425600 - 26700) [02839]; Min I = 2429219.467 +
EQ    Ori    1.74611d*E (JD2427700 - 31000) [00001];
EQ    Ori    since JD2431000 - see Table.
ER    Ori    VB A (B 13.6", 0deg). Min II 9.97. P var. Min I =
ER    Ori    2426336.6485 + 0.4233955d*E (JD2426330 - 33920)
ER    Ori    [00279]; Min I = 2434765.6306 + 0.42340620d*E
ER    Ori    (JD2433920 - 35475) [02278]; Min I = 2436508.7851 +
ER    Ori    0.4234009d*E (JD2435475 - 40000) [03787];
ER    Ori    since JD2440000 - see Table. Shape of the light curve
ER    Ori    varies.
ET    Ori    Min II 11.3. P var?
EW    Ori    Min II 10.5; Min II - Min I = 0.529P.
EW    Ori    In the region of the open cluster CR 70.
EW    Ori    In [00007] Min II are accepted to be Min I, and vice
EW    Ori    versa (Min II - Min I = 0.47P).
EW    Ori    For decisive choice of the Min I epoch photoelectric
EW    Ori    observations are necessary. P var? Min II =
EW    Ori    2429974.810 + 6.9368005d*E [00007]; since
EW    Ori    JD2430000 - see Table.
EY    Ori    Min II 9.54; d = 0.003P. In the region of the Orion
EY    Ori    nebula T-association. P var.
EY    Ori    Min I = 2427310.420 + 16.787450d*E [00007];
EY    Ori    since JD2427500 - see Table.
EZ    Ori    In the region of the Orion nebula T-association.
FF    Ori    Min II 10.3.
FH    Ori    d = 0.035P. P var.
FI    Ori    VB A (B 10.5m, 5", 323deg).
FI    Ori    Shape of the light curve varies, probably periodically
FI    Ori    [03790, 05475].
FK    Ori    P var. Min = 2427773.390 + 1.947447d*E (JD2426900 -
FK    Ori    37500); since JD2437500 - see Table.
FL    Ori    P var. Min = 2427452.271 + 1.550971d*E (JD2427450 -
FL    Ori    29600) [03115]; Min = 2430400.649 + 1.55093d*E
FL    Ori    (JD2429600 - 30400);Min = 2432517.755 + 1.550991d*E
FL    Ori    (JD2430400 - 32900); Min = 2434459.571 + 1.550965d*E
FL    Ori    (JD2432900 - 35050); Min = 2436649.568 + 1.550995d*E
FL    Ori    (JD2435050 - 40600); since JD2440600 - see Table.
FO    Ori    Min II 9.7; d = 0.005P.
FR    Ori    Min II 11.1.
FT    Ori    Min II 9.60; DII = 0.08P; Min II - Min I = 0.73P. P var.
FT    Ori    Min I = 2433009.553 + 3.150404d*E (JD2426380 - 38000)
FT    Ori    [02758]; since JD2438000 - see Table.
FT    Ori    The period of apsidal motion 520 +- 100 years [07358].
FU    Ori    Member of FU Ori T-association. In the dark globule B35.
FU    Ori    Connected with a bright cometary nebula and the bright
FU    Ori    hydrogen nebula S 280. Light maximum was in summer
FU    Ori    1937. IN 1980 - 10.6m B.
FZ    Ori    Min II 11.2.
GG    Ori    Min II 11.1; Min II - Min I = 0.427P.
GP    Ori    SC 7/8- .
GQ    Ori    VB A (B 9.7m, 31", 324deg).
GW    Ori    In the T-association CO Ori.
GX    Ori    In the T-association CO - Ori.
GY    Ori    In the T-association CO - Ori.
GZ    Ori    In the region of the Orion nebula T-association.
HH    Ori    In the region of the Orion nebula T-association.
HI    Ori    In the T-association CO - Ori.
HK    Ori    In the T-association CO - Ori.
HK    Ori    Connected with a bright cometary nebula. CO, CH, OH
HK    Ori    emission.
HL    Ori    In the region of the Orion nebula T-association.
HM    Ori    In the T-association CO - Ori.
HN    Ori    In the region of the Orion nebula T-association.
HO    Ori    In the region of the Orion nebula T-association.
HP    Ori    In the region of the Orion nebula T-association.
HQ    Ori    In the region of the Orion nebula T-association.
HR    Ori    In the region of the Orion nebula T-association.
HS    Ori    In the region of the Orion nebula T-association.
HT    Ori    In the region of the Orion nebula T-association.
HU    Ori    In the region of the Orion nebula T-association.
HV    Ori    In the region of the Orion nebula T-association.
HW    Ori    In the region of the Orion nebula T-association.
HX    Ori    In the region of the Orion nebula T-association.
HY    Ori    In the region of the Orion nebula T-association.
HZ    Ori    In the region of the Orion nebula T-association.
II    Ori    In the region of the Orion nebula T-association.
IK    Ori    In the region of the Orion nebula T-association.
IL    Ori    In the region of the Orion nebula T-association.
IM    Ori    In the region of the Orion nebula T-association.
IN    Ori    In the region of the Orion nebula T-association.
IO    Ori    In the region of the Orion nebula T-association.
IP    Ori    In the region of the Orion nebula T-association.
IQ    Ori    In the region of the Orion nebula T-association.
IR    Ori    In the region of the Orion nebula T-association.
IS    Ori    In the region of the Orion nebula T-association.
IT    Ori    In the region of the Orion nebula T-association.
IU    Ori    In the region of the Orion nebula T-association.
IV    Ori    In the region of the Orion nebula T-association.
IW    Ori    In the region of the Orion nebula T-association.
IX    Ori    In the region of the Orion nebula T-association.
IY    Ori    In the region of the Orion nebula T-association.
IZ    Ori    In the region of the Orion nebula T-association.
KK    Ori    In the region of the Orion nebula T-association.
KL    Ori    In the region of the Orion nebula T-association.
KM    Ori    In the region of the Orion nebula T-association.
KN    Ori    In the region of the Orion nebula T-association.
KO    Ori    In the region of the Orion nebula T-association.
KP    Ori    In the region of the Orion nebula T-association.
KQ    Ori    In the region of the Orion nebula T-association.
KR    Ori    In the region of the Orion nebula T-association.
KS    Ori    In the region of the Orion nebula T-association.
KT    Ori    In the region of the Orion nebula T-association.
KU    Ori    In the region of the Orion nebula T-association.
KV    Ori    In the region of the Orion nebula T-association.
KW    Ori    In the region of the Orion nebula T-association.
KX    Ori    In the region of the Orion nebula T-association.
KY    Ori    In the region of the Orion nebula T-association.
KZ    Ori    In the region of the Orion nebula T-association.
LL    Ori    In the region of the Orion nebula T-association.
LM    Ori    In the region of the Orion nebula T-association.
LN    Ori    In the region of the Orion nebula T-association.
LO    Ori    In the region of the Orion nebula T-association.
LP    Ori    In the region of the Orion nebula T-association.
LQ    Ori    In the region of the Orion nebula T-association.
LR    Ori    In the region of the Orion nebula T-association.
LS    Ori    In the region of the Orion nebula T-association.
LT    Ori    In the region of the Orion nebula T-association.
LU    Ori    In the region of the Orion nebula T-association.
LV    Ori    In the region of the Orion nebula T-association.
LW    Ori    In the region of the Orion nebula T-association.
LX    Ori    In the region of the Orion nebula T-association.
LY    Ori    In the region of the Orion nebula T-association.
LZ    Ori    VB B (A 10.3m; B 14.1", 219deg). In the region of the
LZ    Ori    Orion nebula T-association.
MM    Ori    In the region of the Orion nebula T-association.
MN    Ori    In the region of the Orion nebula T-association.
MO    Ori    In the region of the Orion nebula T-association.
MP    Ori    In the region of the Orion nebula T-association.
MQ    Ori    In the region of the Orion nebula T-association.
MR    Ori    In the region of the Orion nebula T-association.
MS    Ori    In the region of the Orion nebula T-association.
MT    Ori    In the region of the Orion nebula T-association.
MU    Ori    In the region of the Orion nebula T-association.
MV    Ori    In the region of the Orion nebula T-association.
MW    Ori    In the region of the Orion nebula T-association.
MX    Ori    In the region of the Orion nebula T-association.
MY    Ori    In the region of the Orion nebula T-association.
MZ    Ori    In the region of the Orion nebula T-association.
NN    Ori    In the region of the Orion nebula T-association.
NO    Ori    In the region of the Orion nebula T-association.
NP    Ori    In the region of the Orion nebula T-association.
NQ    Ori    In the region of the Orion nebula T-association.
NR    Ori    In the region of the Orion nebula T-association.
NS    Ori    In the region of the Orion nebula T-association.
NT    Ori    In the region of the Orion nebula T-association.
NU    Ori    In the region of the Orion nebula T-association. In the
NU    Ori    nebula NGC 1982. Dust shell.
NV    Ori    In the region of the Orion nebula T-association.
NW    Ori    In the region of the Orion nebula T-association.
NX    Ori    In the region of the Orion nebula T-association.
NY    Ori    VB B (A = V566 Ori; B 5", 135deg). In the region of the
NY    Ori    Orion nebula T-association.
NZ    Ori    In the region of the Orion nebula T-association.
OO    Ori    In the region of the Orion nebula T-association.
OP    Ori    In the region of the Orion nebula T-association.
OQ    Ori    In the region of the Orion nebula T-association.
OR    Ori    In the region of the Orion nebula T-association.
OT    Ori    In the region of the Orion nebula T-association.
OU    Ori    In the region of the Orion nebula T-association.
OV    Ori    In the region of the Orion nebula T-association.
OW    Ori    In the region of the Orion nebula T-association.
OX    Ori    In the region of the Orion nebula T-association.
OY    Ori    In the region of the Orion nebula T-association.
OZ    Ori    In the region of the Orion nebula T-association.
PP    Ori    In the region of the Orion nebula T-association.
PQ    Ori    In the region of the nebula IC 434.
PR    Ori    In the region of the Orion nebula T-association.
PS    Ori    In the region of the Orion nebula T-association.
PT    Ori    In the region of the Orion nebula T-association.
PU    Ori    In the region of the nebula IC 434.
PV    Ori    In the region of the Orion nebula T-association.
PW    Ori    In the region of the Orion nebula T-association.
PX    Ori    Vr =  + 298 km/s [09511]. In the region of the Orion
PX    Ori    nebula T-association.
PY    Ori    In the region of the Orion nebula T-association.
PZ    Ori    In the region of the Orion nebula T-association.
QQ    Ori    In the region of the Orion nebula T-association.
QR    Ori    In the region of T-association FU Ori.
QT    Ori    P var? Elements given in the Table are valid in the
QT    Ori    interval JD2429640 - 35550.
V0340 Ori    Epoch of Min brightness is given.
V0343 Ori    Min II 11.0. Shape of the light curve and depth of
V0343 Ori    Min II vary.
V0347 Ori    In the region of the Orion nebula T-association.
V0348 Ori    In the region of the Orion nebula T-association.
V0349 Ori    In the region of the Orion nebula T-association.
V0353 Ori    In the region of the Orion nebula T-association.
V0354 Ori    In the region of the Orion nebula T-association.
V0355 Ori    In the region of the Orion nebula T-association.
V0356 Ori    In the region of the Orion nebula T-association.
V0357 Ori    In the region of the Orion nebula T-association.
V0358 Ori    In the region of the Orion nebula T-association.
V0359 Ori    In the region of the Orion nebula T-association.
V0359 Ori    Epoch of Min HEI line intensity is given.
V0359 Ori    According to [09512], P = 14.612d.
V0360 Ori    In the region of the Orion nebula T-association.
V0361 Ori    VB C (A 4.8m; B 6.1m, 52.4", 93deg; C 129", 97deg).
V0361 Ori    In the region of the Orion nebula T-association.
V0362 Ori    In the region of the Orion nebula T-association.
V0363 Ori    In the region of the Orion nebula T-association.
V0364 Ori    In the region of the Orion nebula T-association.
V0365 Ori    In the region of the Orion nebula T-association.
V0366 Ori    In the region of the Orion nebula T-association.
V0367 Ori    In the region of the Orion nebula T-association.
V0368 Ori    In the region of the Orion nebula T-association.
V0369 Ori    In the region of the Orion nebula T-association.
V0370 Ori    In the T-association CO - Ori.
V0371 Ori    mu = 0.28", ro = 238deg.
V0372 Ori    In the region of the Orion nebula T-association.
V0373 Ori    In the region of the Orion nebula T-association.
V0374 Ori    In the region of the Orion nebula T-association.
V0375 Ori    In the region of the Orion nebula T-association.
V0376 Ori    In the region of the Orion nebula T-association.
V0377 Ori    In the region of the Orion nebula T-association.
V0378 Ori    In the region of the Orion nebula T-association.
V0379 Ori    In the region of the Orion nebula T-association.
V0380 Ori    In the nebula NGC 1999. In the region of the Orion
V0380 Ori    nebula T-association. Spectrum description
V0380 Ori    [04002]. OH, CH emission.
V0381 Ori    In the region of the Orion nebula T-association.
V0382 Ori    P var. MAX = 2431146 + 227.8d*E (JD2429300 - 31200);
V0382 Ori    Mean period is given in the Table (JD2428100 - 33700).
V0383 Ori    In the region of the Orion nebula T-association.
V0384 Ori    In the region of the Orion nebula T-association.
V0385 Ori    In the region of the Orion nebula T-association.
V0386 Ori    In the region of the Orion nebula T-association.
V0387 Ori    In the region of the Orion nebula T-association.
V0388 Ori    In the region of the Orion nebula T-association.
V0389 Ori    In the region of the Orion nebula T-association.
V0390 Ori    In the region of the Orion nebula T-association.
V0391 Ori    In the region of the Orion nebula T-association.
V0393 Ori    In the region of the Orion nebula T-association.
V0394 Ori    In the region of the Orion nebula T-association.
V0395 Ori    In the region of the Orion nebula T-association.
V0396 Ori    In the region of the Orion nebula T-association.
V0397 Ori    In the region of the Orion nebula T-association.
V0398 Ori    In the region of the Orion nebula T-association.
V0399 Ori    In the region of the Orion nebula T-association.
V0400 Ori    In the region of the Orion nebula T-association.
V0401 Ori    In the region of the Orion nebula T-association.
V0402 Ori    In the region of the Orion nebula T-association.
V0403 Ori    In the region of the Orion nebula T-association.
V0404 Ori    In the region of the Orion nebula T-association.
V0405 Ori    In the region of the Orion nebula T-association.
V0406 Ori    In the region of the Orion nebula T-association.
V0407 Ori    In the region of the Orion nebula T-association.
V0408 Ori    In the region of the Orion nebula T-association.
V0409 Ori    In the region of the Orion nebula T-association.
V0410 Ori    In the region of the Orion nebula T-association.
V0411 Ori    In the region of the Orion nebula T-association.
V0412 Ori    In the region of the Orion nebula T-association.
V0413 Ori    In the region of the Orion nebula T-association.
V0414 Ori    In the region of the Orion nebula T-association.
V0415 Ori    In the region of the Orion nebula T-association.
V0416 Ori    In the region of the Orion nebula T-association.
V0417 Ori    In the region of the Orion nebula T-association.
V0418 Ori    In the region of the Orion nebula T-association.
V0419 Ori    In the region of the Orion nebula T-association.
V0420 Ori    In the region of the Orion nebula T-association.
V0421 Ori    In the region of the Orion nebula T-association.
V0422 Ori    In the region of the Orion nebula T-association.
V0423 Ori    In the region of the Orion nebula T-association.
V0424 Ori    In the region of the Orion nebula T-association.
V0425 Ori    In the region of the Orion nebula T-association.
V0426 Ori    In the region of the Orion nebula T-association.
V0427 Ori    In the region of the Orion nebula T-association.
V0428 Ori    In the region of the Orion nebula T-association.
V0432 Ori    Delta(S) = 0.
V0435 Ori    P var. Max = 2430350 + 186d*E (JD2429600 - 30730);
V0435 Ori    Max = 2431373 + 186d*E (JD2431370 - 3250) [02279];
V0435 Ori    since JD2434000 - see Table.
V0436 Ori    In the T-association CO Ori.
V0437 Ori    In the T-association CO Ori.
V0438 Ori    In the T-association CO Ori.
V0439 Ori    In the T-association CO Ori.
V0441 Ori    In the T-association CO Ori.
V0442 Ori    VB A (B 16.6m, 20", 73deg). In the T-association CO Ori.
V0443 Ori    In the T-association CO Ori.
V0444 Ori    In the T-association CO Ori.
V0445 Ori    In the T-association CO Ori.
V0446 Ori    In the T-association CO Ori.
V0447 Ori    In the T-association CO Ori.
V0448 Ori    In the T-association CO Ori.
V0449 Ori    In the T-association CO Ori.
V0449 Ori    In [08289] was considered as an EW type variable with the
V0449 Ori    elements: Min I = 2430259.622 + 0.441990d*E
V0449 Ori    (JD2430250 - 5550), 14.8m - 15.7m pg.
V0450 Ori    In the T-association CO Ori.
V0452 Ori    In the T-association CO Ori.
V0453 Ori    In the T-association CO Ori.
V0454 Ori    In the T-association CO Ori.
V0455 Ori    In the T-association CO Ori.
V0456 Ori    In the T-association CO Ori.
V0457 Ori    In the T-association CO Ori.
V0458 Ori    In the T-association CO Ori.
V0460 Ori    In the T-association CO Ori.
V0461 Ori    In the T-association CO Ori.
V0463 Ori    In the T-association CO Ori.
V0464 Ori    In the T-association CO Ori.
V0465 Ori    In the T-association CO Ori.
V0466 Ori    In the region of the Orion nebula T-association.
V0467 Ori    In the T-association CO Ori.
V0468 Ori    In the region of the Orion nebula T-association.
V0470 Ori    In the region of the Orion nebula T-association. Star
V0470 Ori    Pi 1411. Near to WY Ori = Pi 1396.
V0473 Ori    In the region of the Orion nebula T-association.
V0474 Ori    In the region of the Orion nebula T-association.
V0475 Ori    In the region of the Orion nebula T-association.
V0476 Ori    In the region of the open cluster lambda Ori.
V0477 Ori    In the region of the open cluster lambda Ori.
V0478 Ori    In the region of the Orion nebula T-association.
V0479 Ori    In the region of the Orion nebula T-association. In the
V0479 Ori    infrared A>1.5m.
V0480 Ori    In the region of the Orion nebula T-association. In the
V0480 Ori    infrared A>1.5m.
V0481 Ori    In the region of the Orion nebula T-association.
V0482 Ori    In the region of the Orion nebula T-association.
V0484 Ori    In the region of the Orion nebula T-association.
V0484 Ori    In the infrared A>1.0m.
V0485 Ori    In the region of the Orion nebula T-association.
V0485 Ori    In the infrared  A>1.0m.
V0486 Ori    In the region of the Orion nebula T-association.
V0487 Ori    In the region of the Orion nebula T-association.
V0489 Ori    In the region of the Orion nebula T-association.
V0489 Ori    In the infrared A>1.0m.
V0490 Ori    In the region of the Orion nebula T-association.
V0490 Ori    In the infrared A>1.0m.
V0491 Ori    In the region of the Orion nebula T-association.
V0491 Ori    In the infrared A>1.0m.
V0492 Ori    In the region of the Orion nebula T-association.
V0492 Ori    Northern component of the close pair of infrared stars.
V0492 Ori    In the infrared A = 1m.
V0493 Ori    In the region of the Orion nebula T-association.
V0493 Ori    In the infrared A>1.0m.
V0494 Ori    In the region of the Orion nebula T-association.
V0495 Ori    In the region of the Orion nebula T-association.
V0495 Ori    Close binary (ro = 0.24"). It is unknown which of the
V0495 Ori    components varies.
V0496 Ori    In the region of the Orion nebula T-association.
V0496 Ori    In the infrared A>1.0m.
V0497 Ori    In the region of the Orion nebula T-association.
V0497 Ori    In the infrared A>1.0m.
V0498 Ori    In the region of the Orion nebula T-association.
V0500 Ori    In the region of the Orion nebula T-association.
V0501 Ori    In the region of the Orion nebula T-association.
V0502 Ori    In the region of the Orion nebula T-association.
V0504 Ori    Min II 15.4.
V0505 Ori    In the region of the nebula IC 434.
V0507 Ori    In the region of the nebula IC 434.
V0508 Ori    In the region of the nebula IC 434.
V0509 Ori    In the region of the nebula IC 434.
V0510 Ori    In the region of the nebula IC 434.
V0511 Ori    In the region of the nebula IC 434.
V0514 Ori    In the region of the nebula IC 434.
V0516 Ori    Max = 2430325 + 139d*E (JD2430250 - 5350); P = 70d
V0516 Ori    (JD2435350 - 550).
V0519 Ori    Min II 12.9.
V0522 Ori    In the region of the nebula IC 434.
V0523 Ori    In the region of the nebula IC 434.
V0525 Ori    Min II 14.7.
V0526 Ori    In the region of T-association FU Ori.
V0529 Ori    Nova Ori 1678?
V0529 Ori    Recurrent outburst was possibly observed at 1894 [02866].
V0529 Ori    Earlier the object was considered as nova Ori [1667
V0529 Ori    2862, 2863, 2867, 2868], its existence being considered
V0529 Ori    as doubtful [03813].
V0537 Ori    In the region of the open cluster lambda Ori.
V0538 Ori    In the region of the Orion nebula T-association.
V0539 Ori    In the region of the Orion nebula T-association.
V0540 Ori    In the region of the Orion nebula T-association.
V0541 Ori    In the region of the Orion nebula T-association.
V0542 Ori    In the region of the Orion nebula T-association.
V0544 Ori    In the region of the Orion nebula T-association.
V0545 Ori    In the region of the Orion nebula T-association.
V0546 Ori    In the region of the Orion nebula T-association.
V0547 Ori    In the region of the Orion nebula T-association.
V0548 Ori    In the region of the open cluster lambda Ori.
V0549 Ori    In the region of the open cluster lambda Ori.
V0550 Ori    In the region of the Orion nebula T-association.
V0551 Ori    In the region of the Orion nebula T-association.
V0552 Ori    In the region of the Orion nebula T-association.
V0553 Ori    In the region of the Orion nebula T-association.
V0554 Ori    In the region of the Orion nebula T-association.
V0555 Ori    In the region of the Orion nebula T-association.
V0556 Ori    In the region of the Orion nebula T-association.
V0557 Ori    In the region of the Orion nebula T-association.
V0559 Ori    In the region of the Orion nebula T-association.
V0560 Ori    In the region of the Orion nebula T-association.
V0561 Ori    In the region of the Orion nebula T-association.
V0562 Ori    In the region of the Orion nebula T-association.
V0563 Ori    In the region of the Orion nebula T-association.
V0564 Ori    In the region of the Orion nebula T-association.
V0565 Ori    In the region of the Orion nebula T-association.
V0566 Ori    In the region of the Orion nebula T-association.
V0567 Ori    In the region of the Orion nebula T-association.
V0568 Ori    In the region of the Orion nebula T-association.
V0569 Ori    In the region of the Orion nebula T-association.
V0570 Ori    In the region of the Orion nebula T-association.
V0571 Ori    In the region of the Orion nebula T-association.
V0572 Ori    In the region of the open cluster lambda Ori.
V0573 Ori    In the region of the Orion nebula T-association.
V0574 Ori    In the region of the Orion nebula T-association.
V0575 Ori    In the region of the Orion nebula T-association.
V0576 Ori    In the region of the Orion nebula T-association.
V0577 Ori    In the region of the Orion nebula T-association.
V0578 Ori    In the region of the Orion nebula T-association.
V0579 Ori    In the region of the Orion nebula T-association.
V0580 Ori    In the region of the Orion nebula T-association.
V0581 Ori    In the region of the Orion nebula T-association.
V0582 Ori    In the region of the Orion nebula T-association.
V0584 Ori    In the region of the Orion nebula T-association.
V0585 Ori    In the region of the Orion nebula T-association.
V0586 Ori    In the region of the Orion nebula T-association.
V0587 Ori    In the region of the Orion nebula T-association.
V0588 Ori    In the region of the Orion nebula T-association.
V0589 Ori    In the region of the Orion nebula T-association.
V0590 Ori    In the region of the Orion nebula T-association.
V0591 Ori    In the region of the Orion nebula T-association.
V0592 Ori    In the region of the Orion nebula T-association.
V0593 Ori    In the region of the Orion nebula T-association.
V0594 Ori    In the region of the Orion nebula T-association.
V0595 Ori    In the region of the nebula IC 434.
V0596 Ori    In the region of the open cluster lambda Ori.
V0597 Ori    In the region of the nebula IC 434.
V0598 Ori    In the region of the open cluster lambda Ori.
V0599 Ori    In the region of the Orion nebula T-association.
V0600 Ori    In the region of the nebula IC 434.
V0601 Ori    In the region of the nebula IC 434.
V0602 Ori    In the region of the nebula IC 434.
V0603 Ori    In the region of the nebula IC 434.
V0604 Ori    In the region of the nebula IC 434.
V0605 Ori    In the region of the nebula IC 434.
V0606 Ori    In the region of the nebula IC 434.
V0607 Ori    In the region of the nebula IC 434.
V0608 Ori    In the region of the nebula IC 434.
V0610 Ori    In the region of the nebula IC 434.
V0611 Ori    In the region of the nebula IC 434.
V0612 Ori    VB, SE-comp.; NW-comp.=NSV 02555. In the region of the
V0612 Ori    nebula IC 434.
V0614 Ori    In the region of T-association FU Ori.
V0615 Ori    In the region of the nebula IC 434.
V0616 Ori    In the region of the nebula IC 434.
V0617 Ori    In the region of the nebula IC 434.
V0618 Ori    In the region of the nebula IC 434.
V0619 Ori    In the region of the nebula IC 434.
V0620 Ori    In the region of the nebula IC 434.
V0621 Ori    In the region of the nebula IC 434.
V0622 Ori    In the region of the nebula IC 434.
V0623 Ori    In the region of the nebula IC 434.
V0625 Ori    In the region of T-association FU Ori.
V0626 Ori    In the region of T-association FU Ori.
V0627 Ori    In the region of T-association FU Ori.
V0628 Ori    In the region of T-association FU Ori.
V0629 Ori    In the region of T-association FU Ori.
V0630 Ori    In the region of T-association FU Ori.
V0631 Ori    In the region of T-association FU Ori.
V0632 Ori    In the region of T-association FU Ori.
V0634 Ori    In the region of T-association FU Ori.
V0635 Ori    In the region of T-association FU Ori.
V0636 Ori    In the region of T-association FU Ori.
V0637 Ori    In the region of T-association FU Ori.
V0638 Ori    In the region of T-association FU Ori.
V0639 Ori    In the region of T-association FU Ori.
V0640 Ori    d <= 0.02P.
V0641 Ori    Min II 14.5.
V0642 Ori    d = 0.05P?.
V0643 Ori    P = 26.2075d?
V0647 Ori    Min II 11.9. P var. Min I = 2418005.035 + 0.977575d*E
V0647 Ori    (JD2414660 - 23230); since JD2423230 - see Table.
V0648 Ori    Min II 12.2.
V0649 Ori    In the T-association CO - Ori. VB A (B 15m, 2", 0deg).
V0650 Ori    In the region of the open cluster lambda Ori.
V0652 Ori    In the region of the Orion nebula T-association.
V0654 Ori    In the region of the Orion nebula T-association.
V0655 Ori    In the region of the Orion nebula T-association.
V0656 Ori    In the region of the Orion nebula T-association.
V0657 Ori    In the region of the Orion nebula T-association.
V0658 Ori    In the region of the Orion nebula T-association.
V0659 Ori    In the region of the Orion nebula T-association.
V0667 Ori    Min II 15.0.
V0676 Ori    In the region of the Orion nebula T-association.
V0677 Ori    In the region of the Orion nebula T-association.
V0678 Ori    In the region of the Orion nebula T-association.
V0679 Ori    In the region of the Orion nebula T-association.
V0680 Ori    In the region of the Orion nebula T-association.
V0681 Ori    In the region of the Orion nebula T-association.
V0682 Ori    In the region of the Orion nebula T-association.
V0683 Ori    In the region of the Orion nebula T-association.
V0684 Ori    In the region of the Orion nebula T-association.
V0685 Ori    In the region of the Orion nebula T-association.
V0685 Ori    A(U) = 1.0m.
V0686 Ori    In the region of the Orion nebula T-association.
V0687 Ori    In the region of the Orion nebula T-association.
V0688 Ori    In the region of the Orion nebula T-association.
V0689 Ori    In the region of the Orion nebula T-association.
V0690 Ori    In the region of the Orion nebula T-association.
V0691 Ori    In the region of the Orion nebula T-association.
V0692 Ori    In the region of the Orion nebula T-association.
V0693 Ori    In the region of the Orion nebula T-association.
V0694 Ori    In the region of the Orion nebula T-association.
V0695 Ori    In the region of the Orion nebula T-association.
V0696 Ori    In the region of the Orion nebula T-association.
V0697 Ori    In the region of the Orion nebula T-association.
V0698 Ori    In the region of the Orion nebula T-association.
V0699 Ori    In the region of the Orion nebula T-association.
V0700 Ori    In the region of the Orion nebula T-association.
V0701 Ori    In the region of the Orion nebula T-association.
V0702 Ori    In the region of the Orion nebula T-association.
V0703 Ori    In the region of the Orion nebula T-association.
V0704 Ori    In the region of the Orion nebula T-association.
V0705 Ori    In the region of the Orion nebula T-association.
V0706 Ori    In the region of the Orion nebula T-association.
V0707 Ori    In the region of the Orion nebula T-association.
V0708 Ori    In the region of the Orion nebula T-association.
V0709 Ori    In the region of the Orion nebula T-association.
V0710 Ori    In the region of the Orion nebula T-association.
V0711 Ori    In the region of the Orion nebula T-association.
V0712 Ori    In the region of the Orion nebula T-association.
V0713 Ori    In the region of the Orion nebula T-association.
V0713 Ori    A(U) = 4.0m.
V0714 Ori    In the region of the Orion nebula T-association.
V0715 Ori    In the region of the Orion nebula T-association.
V0716 Ori    In the region of the Orion nebula T-association.
V0717 Ori    In the region of the Orion nebula T-association.
V0718 Ori    In the region of the Orion nebula T-association.
V0718 Ori    Probably the sf-component of a very close pair.
V0719 Ori    In the region of the Orion nebula T-association.
V0720 Ori    In the region of the Orion nebula T-association.
V0721 Ori    In the region of the Orion nebula T-association.
V0722 Ori    In the region of the Orion nebula T-association.
V0723 Ori    In the region of the Orion nebula T-association.
V0724 Ori    In the region of the Orion nebula T-association.
V0725 Ori    In the region of the Orion nebula T-association.
V0726 Ori    In the region of the Orion nebula T-association.
V0727 Ori    In the region of the Orion nebula T-association.
V0728 Ori    In the region of the Orion nebula T-association.
V0729 Ori    In the region of the Orion nebula T-association.
V0730 Ori    In the region of the Orion nebula T-association.
V0731 Ori    In the region of the Orion nebula T-association.
V0732 Ori    In the region of the Orion nebula T-association.
V0733 Ori    In the region of the Orion nebula T-association.
V0734 Ori    In the region of the Orion nebula T-association.
V0735 Ori    In the region of the Orion nebula T-association.
V0736 Ori    In the region of the Orion nebula T-association.
V0737 Ori    In the region of the Orion nebula T-association.
V0737 Ori    A(U) > 2.4m.
V0738 Ori    In the region of the Orion nebula T-association.
V0739 Ori    In the region of the Orion nebula T-association.
V0740 Ori    In the region of the Orion nebula T-association.
V0740 Ori    A(pg) > 4.0m.
V0741 Ori    In the region of the Orion nebula T-association.
V0742 Ori    In the region of the Orion nebula T-association.
V0744 Ori    In the region of the Orion nebula T-association.
V0745 Ori    In the region of the Orion nebula T-association.
V0746 Ori    In the region of the Orion nebula T-association.
V0747 Ori    In the region of the Orion nebula T-association.
V0748 Ori    In the region of the Orion nebula T-association.
V0749 Ori    In the region of the Orion nebula T-association.
V0750 Ori    In the region of the Orion nebula T-association.
V0751 Ori    In the region of the Orion nebula T-association.
V0752 Ori    In the region of the Orion nebula T-association.
V0753 Ori    In the region of the Orion nebula T-association.
V0754 Ori    In the region of the Orion nebula T-association.
V0755 Ori    In the region of the Orion nebula T-association.
V0756 Ori    In the region of the Orion nebula T-association.
V0757 Ori    In the region of the Orion nebula T-association.
V0758 Ori    In the region of the Orion nebula T-association.
V0759 Ori    In the region of the Orion nebula T-association.
V0760 Ori    In the region of the Orion nebula T-association.
V0761 Ori    In the region of the Orion nebula T-association.
V0762 Ori    In the region of the Orion nebula T-association.
V0763 Ori    In the region of the Orion nebula T-association.
V0764 Ori    In the region of the Orion nebula T-association.
V0765 Ori    In the region of the Orion nebula T-association.
V0766 Ori    In the region of the Orion nebula T-association.
V0767 Ori    In the region of the Orion nebula T-association.
V0767 Ori    A(U) = 1.5m.
V0768 Ori    In the region of the Orion nebula T-association.
V0770 Ori    In the region of the Orion nebula T-association.
V0771 Ori    In the region of the Orion nebula T-association.
V0772 Ori    In the region of the Orion nebula T-association.
V0773 Ori    In the region of the Orion nebula T-association.
V0774 Ori    In the region of the Orion nebula T-association.
V0775 Ori    In the region of the Orion nebula T-association.
V0776 Ori    In the region of the Orion nebula T-association.
V0777 Ori    In the region of the Orion nebula T-association.
V0778 Ori    In the region of the Orion nebula T-association.
V0778 Ori    A(pg) = 1.6m.
V0779 Ori    In the region of the Orion nebula T-association.
V0780 Ori    In the region of the Orion nebula T-association.
V0780 Ori    A(U) = 1.0m.
V0781 Ori    In the region of the Orion nebula T-association.
V0782 Ori    In the region of the Orion nebula T-association.
V0783 Ori    In the region of the Orion nebula T-association.
V0783 Ori    A(pg) = 3.0m.
V0784 Ori    In the region of the Orion nebula T-association.
V0785 Ori    In the region of the Orion nebula T-association.
V0786 Ori    In the region of the Orion nebula T-association.
V0787 Ori    In the region of the Orion nebula T-association.
V0788 Ori    In the region of the Orion nebula T-association.
V0789 Ori    In the region of the Orion nebula T-association.
V0790 Ori    In the region of the Orion nebula T-association.
V0791 Ori    In the region of the Orion nebula T-association.
V0792 Ori    In the region of the Orion nebula T-association.
V0793 Ori    In the region of the Orion nebula T-association.
V0794 Ori    In the region of the Orion nebula T-association.
V0795 Ori    In the region of the Orion nebula T-association.
V0796 Ori    In the region of the Orion nebula T-association.
V0797 Ori    In the region of the Orion nebula T-association.
V0798 Ori    In the region of the Orion nebula T-association.
V0799 Ori    In the region of the Orion nebula T-association.
V0800 Ori    In the region of the Orion nebula T-association.
V0801 Ori    In the region of the Orion nebula T-association.
V0802 Ori    In the region of the Orion nebula T-association.
V0803 Ori    In the region of the Orion nebula T-association.
V0804 Ori    In the region of the Orion nebula T-association.
V0805 Ori    In the region of the Orion nebula T-association.
V0806 Ori    In the region of the Orion nebula T-association.
V0807 Ori    In the region of the Orion nebula T-association.
V0808 Ori    In the region of the Orion nebula T-association.
V0810 Ori    In the region of the Orion nebula T-association.
V0811 Ori    In the region of the Orion nebula T-association.
V0812 Ori    In the region of the Orion nebula T-association.
V0813 Ori    In the region of the Orion nebula T-association.
V0814 Ori    In the region of the Orion nebula T-association.
V0815 Ori    In the region of the Orion nebula T-association.
V0816 Ori    In the region of the Orion nebula T-association.
V0817 Ori    In the region of the Orion nebula T-association.
V0818 Ori    In the region of the Orion nebula T-association.
V0819 Ori    In the region of the Orion nebula T-association.
V0820 Ori    In the region of the Orion nebula T-association.
V0821 Ori    In the region of the Orion nebula T-association.
V0822 Ori    In the region of the Orion nebula T-association.
V0823 Ori    In the region of the Orion nebula T-association.
V0824 Ori    In the region of the Orion nebula T-association.
V0825 Ori    In the region of the Orion nebula T-association.
V0826 Ori    In the region of the Orion nebula T-association.
V0827 Ori    In the region of the Orion nebula T-association.
V0828 Ori    In the region of the Orion nebula T-association.
V0829 Ori    In the region of the Orion nebula T-association.
V0830 Ori    In the region of the Orion nebula T-association.
V0831 Ori    In the region of the Orion nebula T-association.
V0832 Ori    In the region of the Orion nebula T-association.
V0833 Ori    In the region of the Orion nebula T-association.
V0834 Ori    In the region of the Orion nebula T-association.
V0835 Ori    In the region of the Orion nebula T-association.
V0836 Ori    In the region of the Orion nebula T-association.
V0836 Ori    A(U) > 1.5m.
V0837 Ori    In the region of the Orion nebula T-association.
V0838 Ori    In the region of tbe Orion nebula T-association.
V0839 Ori    In the region of tbe Orion nebula T-association.
V0840 Ori    In the region of the Orion nebula T-association.
V0840 Ori    A(pg) = 0.7m.
V0841 Ori    In the region of the Orion nebula T-association.
V0842 Ori    In the region of the Orion nebula T-association.
V0843 Ori    In the region of the Orion nebula T-association.
V0844 Ori    In the region of the Orion nebula T-association.
V0845 Ori    In the region of the Orion nebula T-association.
V0846 Ori    In the region of the Orion nebula T-association.
V0847 Ori    In the region of the Orion nebula T-association.
V0848 Ori    In the region of the Orion nebula T-association.
V0849 Ori    In the region of the Orion nebula T-association.
V0850 Ori    In the region of the Orion nebula T-association.
V0851 Ori    In the region of the Orion nebula T-association.
V0852 Ori    In the region of the Orion nebula T-association.
V0853 Ori    In the region of the Orion nebula T-association.
V0854 Ori    In the region of the Orion nebula T-association.
V0855 Ori    In the region of the Orion nebula T-association.
V0855 Ori    A(U) > 2.0m.
V0856 Ori    In the region of the Orion nebula T-association.
V0857 Ori    In the region of the Orion nebula T-association.
V0857 Ori    A(pg) > 5.0m.
V0858 Ori    In the region of the Orion nebula T-association.
V0859 Ori    In the region of the Orion nebula T-association.
V0860 Ori    In the region of the Orion nebula T-association.
V0861 Ori    In the region of the Orion nebula T-association.
V0862 Ori    In the region of the Orion nebula T-association.
V0863 Ori    In the region of the Orion nebula T-association.
V0864 Ori    In the region of the Orion nebula T-association.
V0865 Ori    In the region of the Orion nebula T-association.
V0866 Ori    In the region of the Orion nebula T-association.
V0867 Ori    In the region of the Orion nebula T-association.
V0867 Ori    A(pg)>3.0m.
V0868 Ori    In the region of the Orion nebula T-association.
V0869 Ori    In the region of the Orion nebula T-association.
V0870 Ori    In the region of the Orion nebula T-association.
V0871 Ori    In the region of the Orion nebula T-association.
V0872 Ori    In the region of the Orion nebula T-association.
V0873 Ori    In the region of the Orion nebula T-association.
V0874 Ori    In the region of the Orion nebula T-association.
V0875 Ori    In the region of the Orion nebula T-association.
V0876 Ori    In the region of the Orion nebula T-association.
V0876 Ori    Southem component of a close pair.
V0877 Ori    In the region of the Orion nebula T-association.
V0878 Ori    In the region of the Orion nebula T-association.
V0879 Ori    In the region of the Orion nebula T-association.
V0880 Ori    In the region of the Orion nebula T-association.
V0881 Ori    In the region of the Orion nebula T-association.
V0882 Ori    In the region of the Orion nebula T-association.
V0883 Ori    In the region of the Orion nebula T-association.
V0883 Ori    In the apex of a cometary nebula.
V0884 Ori    In the region of the Orion nebula T-association.
V0885 Ori    In the region of the Orion nebula T-association.
V0886 Ori    In the region of the Orion nebula T-association.
V0886 Ori    A(pg) > 3.5m.
V0888 Ori    In the region of the Orion nebula T-association.
V0889 Ori    In the region of the Orion nebula T-association.
V0890 Ori    In the region of the Orion nebula T-association.
V0891 Ori    In the region of the Orion nebula T-association.
V0892 Ori    In the region of the Orion nebula T-association.
V0892 Ori    Southern component of a pair (ro = 3").
V0893 Ori    In the region of the Orion nebula T-association.
V0893 Ori    A(U) = 2.0m.
V0894 Ori    In the region of the Orion nebula T-association.
V0895 Ori    In the region of the Orion nebula T-association.
V0896 Ori    In the region of the Orion nebula T-association.
V0897 Ori    In the region of the Orion nebula T-association.
V0898 Ori    In the region of the Orion nebula T-association.
V0899 Ori    In the region of the Orion nebula T-association.
V0900 Ori    In the region of the Orion nebula T-association.
V0900 Ori    A(pg) > 2.5m.
V0901 Ori    In the region of the nebula IC 434.
V0902 Ori    In the region of the Orion nebula T-association.
V0904 Ori    In the region of the Orion nebula T-association.
V0905 Ori    In the region of the Orion nebula T-association.
V0906 Ori    In the region of the Orion nebula T-association.
V0907 Ori    In the region of the Orion nebula T-association.
V0908 Ori    In the region of the Orion nebula T-association.
V0909 Ori    In the region of the Orion nebula T-association.
V0916 Ori    P = 0.28297d? Member of the open cluster NGC 2169.
V0917 Ori    Member of the open cluster NGC 2169.
V0918 Ori    In the region of the Orion nebula T-association.
V0919 Ori    In the region of the Orion nebula T-association.
V0920 Ori    In the region of the Orion nebula T-association.
V0921 Ori    In the region of the Orion nebula T-association.
V0922 Ori    In the region of the Orion nebula T-association.
V0923 Ori    In the region of the Orion nebula T-association.
V0924 Ori    In the region of the Orion nebula T-association.
V0926 Ori    In the region of the Orion nebula T-association.
V0927 Ori    In the region of the Orion nebula T-association.
V0928 Ori    In the region of the Orion nebula T-association.
V0929 Ori    In the region of the Orion nebula T-association.
V0930 Ori    In the region of the Orion nebula T-association.
V0931 Ori    In the region of the Orion nebula T-association.
V0932 Ori    In the region of the Orion nebula T-association.
V0933 Ori    In the region of the Orion nebula T-association.
V0934 Ori    In the region of the Orion nebula T-association.
V0935 Ori    In the region of the Orion nebula T-association.
V0937 Ori    In the region of the Orion nebula T-association.
V0938 Ori    In the region of the Orion nebula T-association.
V0939 Ori    In the region of the Orion nebula T-association.
V0941 Ori    In the region of the Orion nebula T-association.
V0942 Ori    In the region of the Orion nebula T-association.
V0943 Ori    In the region of the Orion nebula T-association.
V0945 Ori    In the region of the Orion nebula T-association.
V0946 Ori    In the region of the Orion nebula T-association.
V0947 Ori    In the region of the Orion nebula T-association.
V0948 Ori    In the region of the Orion nebula T-association.
V0949 Ori    In the region of the Orion nebula T-association.
V0950 Ori    In the region of the Orion nebula T-association.
V0951 Ori    In the region of the Orion nebula T-association.
V0952 Ori    In the region of the Orion nebula T-association.
V0953 Ori    In the region of the nebula IC 434.
V0956 Ori    In the region of the nebula IC 434.
V0957 Ori    In the region of the nebula IC 434.
V0958 Ori    In the region of the Orion nebula T-association.
V0960 Ori    In the region of the nebula IC 434.
V0961 Ori    In the region of the Orion nebula T-association.
V0964 Ori    P var. Max = 2415800.389 + 0.5046772d*E
V0964 Ori    (JD2415800 - 21010); Max = 2424500.446 + 0.50466477d*E
V0964 Ori    (JD2424500 - 30500); since JD2431500 - see Table.
V0966 Ori    In the region of the Orion nebula T-association.
V0967 Ori    In the region of the Orion nebula T-association.
V0968 Ori    In the region of the Orion nebula T-association.
V0969 Ori    In the region of the Orion nebula T-association.
V0970 Ori    In the region of the Orion nebula T-association.
V0971 Ori    In the region of the Orion nebula T-association.
V0972 Ori    In the region of the Orion nebula T-association.
V0973 Ori    In the region of the Orion nebula T-association.
V0974 Ori    In the region of the Orion nebula T-association.
V0975 Ori    In the region of the Orion nebula T-association.
V0976 Ori    In the region of the Orion nebula T-association.
V0977 Ori    In the region of the Orion nebula T-association.
V0978 Ori    In the region of the Orion nebula T-association.
V0979 Ori    In the region of the Orion nebula T-association.
V0980 Ori    In the region of the Orion nebula T-association.
V0981 Ori    In the region of the Orion nebula T-association.
V0982 Ori    In the region of the Orion nebula T-association.
V0983 Ori    In the region of the Orion nebula T-association.
V0984 Ori    In the region of the Orion nebula T-association.
V0985 Ori    In the region of the Orion nebula T-association.
V0986 Ori    In the region of the Orion nebula T-association.
V0987 Ori    In the region of the Orion nebula T-association.
V0988 Ori    In the region of the Orion nebula T-association.
V0989 Ori    In the region of the Orion nebula T-association.
V0990 Ori    In the region of the Orion nebula T-association.
V0991 Ori    In the region of the Orion nebula T-association.
V0992 Ori    In the region of the Orion nebula T-association.
V0994 Ori    In the region of the Orion nebula T-association.
V0995 Ori    In the region of the Orion nebula T-association.
V0996 Ori    In the region of the Orion nebula T-association.
V0997 Ori    In the region of the Orion nebula T-association.
V0998 Ori    mu = 0.28", ro = 221deg.
V0999 Ori    In the region of the Orion nebula T-association.
V1000 Ori    In the region of the Orion nebula T-association.
V1001 Ori    In the region of the Orion nebula T-association.
V1002 Ori    In the region of the Orion nebula T-association.
V1003 Ori    mu = 0.272", ro = 60.8deg.
V1004 Ori    VB A (B 10.57m, 37", 204deg); SB (P = 2.74d).
V1005 Ori    The range of light variations (characteristic for BY Dra
V1005 Ori    type variability) between the flares is given in the Table;
V1005 Ori    the amplitude of the flares A(U) can reach 3.2m.
V1006 Ori    In the region of the Orion nebula T-association.
V1007 Ori    In the region of the Orion nebula T-association.
V1016 Ori    In the region of the Orion nebula T-association.
V1016 Ori    In the cluster NGC 1976. Orion Trapezium
V1016 Ori    member: teta1 Ori A (B = BM Ori, 8.7", 32deg; C 5.13m,
V1016 Ori    13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.001P.
V1017 Ori    In the region of the Orion nebula T-association.
V1018 Ori    In the region of the Orion nebula T-association.
V1019 Ori    In the region of the Orion nebula T-association.
V1020 Ori    In the region of the Orion nebula T-association.
V1022 Ori    In the region of T-association FU Ori.
V1028 Ori    P = 6d?
V1029 Ori    In the region of the Orion nebula T-association.
V1030 Ori    In the region of the nebula IC 434. (sig Ori) E
V1030 Ori    (A 4.1m; B 5.1m, A = 0.247", P = 170yr; C 8.79m, 11.2",
V1030 Ori    238deg; D 6.66m, 12.9", 84deg; E 41.6", 61deg). Min I
V1030 Ori    (HeI) = 2442802.48 + 1.19080d*E. Unusual helium variable.
V1030 Ori    Epoch of Min I brightness is given in the Table
V1030 Ori    (Min II 6.71, Min II - Min I = 0.43P). This epoch is being
V1030 Ori    observed by 0.18P later than the epoch of minimum strength
V1030 Ori    of the HeI lambda 4026 A line. According to [09524], light
V1030 Ori    minima are due to "eclipses" of the star surface
V1030 Ori    by two isolated clouds (consisting of hydrogen and
V1030 Ori    helium), which are located almost oppositely near
V1030 Ori    the intersections of the magnetic And rotational
V1030 Ori    equator.
V1031 Ori    VB (0.159", 104deg, 1980.7). Min II 6.32; DII = 0.017P.
V1034 Ori    Epoch of light minimum is given.
V1035 Ori    In the region of the Orion nebula T-association.
V1036 Ori    In the region of the Orion nebula T-association.
V1037 Ori    In the region of the Orion nebula T-association.
V1038 Ori    In the region of the Orion nebula T-association.
V1039 Ori    In the region of the Orion nebula T-association.
V1040 Ori    In the region of the Orion nebula T-association.
V1041 Ori    In the region of the Orion nebula T-association.
V1042 Ori    In the region of the Orion nebula T-association.
V1043 Ori    In the region of the Orion nebula T-association.
V1044 Ori    In the region of the Orion nebula T-association.
V1045 Ori    In the region of the Orion nebula T-association.
V1046 Ori    In the region of the Orion nebula T-association.
V1046 Ori    SB 1. Min II 6.58. Possibly an ellipsoidal variable, its
V1046 Ori    light variations being superimposed by light variations of
V1046 Ori    the primary component of SX Ari type:
V1046 Ori    Min (HeI) = 2442812.23 + 0.9015d*E [08054].
V1047 Ori    In the region of the Orion nebula T-association.
V1048 Ori    In the region of the Orion nebula T-association.
V1049 Ori    In the region of the Orion nebula T-association.
V1050 Ori    In the region of the Orion nebula T-association.
V1052 Ori    In the region of the Orion nebula T-association.
V1053 Ori    In the region of the Orion nebula T-association.
V1054 Ori    Epoch of light minimum is given. P = 8.596d?, P = 8.674d?
V1055 Ori    P(X) = 5.2d [09528].
V1056 Ori    VB A (B 9.8m, 28.7", 58deg).
V1058 Ori    In the region of the Orion nebula T-association.
V1059 Ori    In the region of the Orion nebula T-association.
V1060 Ori    In the region of the Orion nebula T-association.
V1061 Ori    In the region of the Orion nebula T-association.
V1062 Ori    In the region of the Orion nebula T-association.
V1063 Ori    In the region of the Orion nebula T-association.
V1064 Ori    In the region of the Orion nebula T-association.
V1065 Ori    In the region of the Orion nebula T-association.
V1066 Ori    In the region of the Orion nebula T-association.
V1067 Ori    In the region of the Orion nebula T-association.
V1068 Ori    In the region of the Orion nebula T-association.
V1069 Ori    In the region of the Orion nebula T-association.
V1070 Ori    In the region of the Orion nebula T-association.
V1071 Ori    In the region of the Orion nebula T-association.
V1072 Ori    In the region of the Orion nebula T-association.
V1073 Ori    In the region of the Orion nebula T-association.
V1074 Ori    In the region of the Orion nebula T-association.
V1075 Ori    In the region of the Orion nebula T-association.
V1076 Ori    In the region of the Orion nebula T-association.
V1077 Ori    In the region of the Orion nebula T-association.
V1078 Ori    In the region of the Orion nebula T-association.
V1079 Ori    In the region of the Orion nebula T-association.
V1080 Ori    In the region of the Orion nebula T-association.
V1081 Ori    In the region of the Orion nebula T-association.
V1082 Ori    In the region of the Orion nebula T-association.
V1083 Ori    In the region of the Orion nebula T-association.
V1084 Ori    In the region of the Orion nebula T-association.
V1377 Ori    SB?, Porb ~ 5.5 to 6.5d.
V1380 Ori    In a bright nebula.
V1647 Ori    The nebula brightened to 14.0, the central star's magnitude is given.
V1650 Ori    The magnitude in Min light is from [130].
V1804 Ori    VB (A 7.7m; B 7.9m, 5", 5deg, 1991).
V1811 Ori    A twice shorter period is not excluded.
V1814 Ori    SB2, Porb = 19.48136d.
V1818 Ori    In the head of the nebula GN 05.51.4.
V1820 Ori    Blazhko effect, P(Bl) = 28d [169].
V1833 Ori    Min II = 10.53. Changing O'Connell effect.
V1834 Ori    Min II = 6.87. VB AB (A 7.0m; B 9.1m, 1".8, 340deg, 2007).
V1840 Ori    VB A (B 13.1m, 13", 211deg, 2001).
V1847 Ori    Amplitude(Min II)=  0.24mag.
V1848 Ori    Min II = 11.65.
V1851 Ori    Min II = 13.05 :.
V1853 Ori    Min II = 12.20 :.
V1859 Ori    SB2, Porb = 5.935d.
V1865 Ori    Min II = 12.8.
V1871 Ori    Min II = 12.9.
V1872 Ori    SB2, Porb = 7.672d.
V1878 Ori    SB2, Porb = 40.57d.
V1882 Ori    SB2, Porb = 46.85d.
V1883 Ori    VB B (A = NEXT GCVS NAME; AB 9", 262deg, 2000).
V1884 Ori    VB A (B = PREVIOUS GCVS NAME, 9", 262deg, 2000).
V1885 Ori    VB AB (1").
V1928 Ori    VB B (A 9.05m; AB 7", 163deg, 2001).
V1931 Ori    VB A (B 13.51m, 8", 359deg, 2001).
V1934 Ori    VB B (A = IM Ori, 12.67m; AB 6", 337deg, 2001).
V1935 Ori    VB A (B 13.88m, 6", 71deg, 2001).
V1952 Ori    VB B (A 10.4m; AB 12", 32deg, 2001).
V1953 Ori    The amplitude of out-of-flare variations is 0.04m.
V1994 Ori    VB B (A = V1000 Ori, 11.70m; AB 6", 194deg, 2001).
V1995 Ori    VB B (A 9.59mJ; B 13.98mJ, 24", 31deg, 2001; C 14.25mJ, BC 7", 214deg, 2001; also other components).
V1999 Ori    Amplitude(Min II)=  0.3mag.
V2008 Ori    VB A (B = V1694 Ori, 12.31mJ, 8", 191deg, 2001).
V2014 Ori    VB AB (7.7mV, 8.2mV, 1".7, 282deg, 2006).
V2024 Ori    VB B (A 13.13m; AB 6", 305deg, 2001).
V2027 Ori    VB A (B 13.87m, 5", 342deg, 2001).
V2030 Ori    VB A (B 16.0m, 5", 133deg, 2001).
V2038 Ori    VB B (A = KK Ori, 11.26m; AB 5", 89deg, 2001).
V2039 Ori    VB A (B 13.11m, 11", 322deg, 2001).
V2084 Ori    VB B (A = NSV 02252, 8.61m; AB 11", 130deg, 2001).
V2085 Ori    VB A (B 12.84m, 10", 36deg).
V2086 Ori    VB B (A = V1474 Ori, 13.30m; AB 19", 291 deg, 2001; C 15.78m; BC 6", 117deg, 2001).
V2088 Ori    VB C (A = V1316 Ori, 12.74m, B 14.40m; AB 8", 353deg, AC 13", 15deg, 2001).
V2090 Ori    VB B (A = V1317 Ori, 14.04m; AB 7", 141deg, 2001).
V2094 Ori    VB A (B 13.20m, 6", 279deg, 2001).
V2099 Ori    Multiple (V1318 Ori 12.75m, 13", 312deg, 2001 and other companions).
V2102 Ori    VB B (A = KS Ori, 9.51m; AB 5", 69deg, 2001).
V2107 Ori    VB A (B = KR Ori, 10.23m; AB 15", 99deg, 2001).
V2109 Ori    VB A (B 12.87m, 5", 353deg, 2001).
V2110 Ori    VB B (A = V1479 Ori, 12.49m; AB 9", 346deg, 2001).
V2113 Ori    VB B (A = NSV 16386, 13.34m; AB 8", 127deg, 2001).
V2114 Ori    VB B (A = V1319 Ori, 10.91m; AB 6", 270deg, 2001).
V2118 Ori    VB B (A 11.54m; AB 11", 218deg, 2001).
V2120 Ori    VB B (A 12.70m; AB 18", 294deg, 2001; C 13.14m; BC 12", 185deg, 2001; D 13.54m; BD 11", 277deg, 2001).
V2121 Ori    VB A (B 13.69m, 5", 309 deg, 2001).
V2133 Ori    VB B (A 8.74m, 20", 346deg, 2001).
V2136 Ori    Type E is not excluded.
V2139 Ori    VB A (B 14.13m, 8", 150deg, 2001).
V2141 Ori    VB A (B 11.64:m, 6", 252deg, 2001).
V2142 Ori    VB B (A 12.72m, 7", 11deg, 2001).
V2143 Ori    VB A (B = V1482 Ori, 12.08m, 10", 274deg, 2001; C = V1322 Ori, 12.11m, 13", 320deg, 2001; D = V1323 Ori, 12.26m, 15", 352deg, 2001).
V2150 Ori    VB B (A = V480 Ori, 11.38m, AB 10", 326deg, 2001; C = GCVS NAME FROM NEXT REMARK, 13.18m, AC 6", 306deg, 2001).
V2152 Ori    VB C (A = V480 Ori, 11.38m, B = GCVS NAME FROM PREVIOUS REMARK; AB 10", 326deg, AC 6", 306deg, 2001).
V2164 Ori    VB B (A 11.53m, K5; AB 10", 189deg, 2001; C 13.44m, M3.5e, AC 5", 153deg, 2001; other components).
V2167 Ori    VB A (B 16.35m, 8", 83deg, 2001).
V2175 Ori    VB A (B = NSV 16405, 13.31m, 9", 106deg, 2001).
V2177 Ori    VB B (A = REMARK AFTER NEXT, 12.96m; AB 4", 238deg, 2001).
V2178 Ori    VB A (B 15.25m, 8", 111deg, 2001).
V2179 Ori    VB A (B = REMARK BEFORE PREVIOUS, 14.72m, 4" 238deg, 2001).
V2181 Ori    VB B (A 12.69m; AB 7", 330deg, 2001).
V2183 Ori    VB B (A 13.36m; AB 8", 111deg, 2001).
V2185 Ori    VB A (B 12.84m, 7", 330deg, 2001).
V2189 Ori    VB B (A 14.43m; AB 6", 297deg, 2001).
V2191 Ori    VB C (A = LR Ori, 9.70m, B 12.92m; AB 10", 160deg, AC 14", 248 deg, 2001; other components).
V2192 Ori    VB B (A 12.88m; AB 6", 317deg, 2001).
V2194 Ori    VB A (B 16.48m, 7", 163deg, 2001).
V2198 Ori    VB B (A 12.04m; AB 5", 65deg, 2001).
V2205 Ori    VB A (B 16.07m, 7", 108deg, 2001).
V2212 Ori    Amplitude(Min II)=  0.1mag.
V2213 Ori    Multiple (V1487 Ori 9.42m, 13". 233deg, 2001; other components, including NSV 16420).
V2214 Ori    VB A (B 13.55m, 11", 118deg, 118deg).
V2215 Ori    VB B (A 12.32m; AB 9", 272deg, 2001; other components).
V2216 Ori    VB A (B 15.54m, 11", 353deg, 2001).
V2217 Ori    Multiple (LU Ori 8.74mKs, 9", 182deg, 2001; other components).
V2218 Ori    VB B (A = LU Ori, 9.98mJ; AB 7", 158deg, 2001).
V2220 Ori    VB A (B 3" s).
V2222 Ori    VB B (A 12.11m; AB 7", 149deg, 2001).
V2225 Ori    Multiple (NSV 16423 14" np; other components).
V2228 Ori    Multiple (NSV 16426 13.58m, 9", 356deg, 2001; GCVS NAME FOR NSV 16429 12.37m, 11", 147deg, 2001; other components).
V2232 Ori    VB A (B 13.64:m, 8", 40deg, 2001; other components).
V2233 Ori    VB B (A = GCVS NAME FOR No. 8384; AB 5", 276deg, 2001).
V2236 Ori    Multiple.
V2237 Ori    VB A (B 12.80m, 6", 123deg, 2001).
V2239 Ori    VB A (B = V1491 Ori, 11.29m, 16", 229deg, 2001).
V2241 Ori    Multiple.
V2242 Ori    VB C (A = GCVS NAME FOR NSV 16438, 12.80m, B = GCVS NAME FOR NSV 16437, 13.37m; AB 13", 191deg, AC 9", 208deg, 2001).
V2243 Ori    VB A (B = GCVS NAME FOR No. 8355, 5", 276deg, 2001).
V2245 Ori    VB B (A = GCVS NAME FOR NSV 16438, 12.80m; AB 13", 191deg, 20001; C = GCVS NAME FOR No. 8381, AC 9", 208deg, 2001).
V2246 Ori    VB A (B 13.24m, 12", 235deg, 2001).
V2247 Ori    VB A (B = GCVS NAME FOR NSV 16437, 13.37m, 13", 191deg, 2001; C = GCVS NAME FOR No. 8381, AC 9", 208deg, 2001).
V2248 Ori    VB A (B = NSV 16441, 8.16:m, 17", 150deg, 2001; C = V1496 Ori, 8.78m, 7", 180deg, 2001).
V2251 Ori    VB C (A 13.52m, B 14.96m; AB 6", 229deg, AC 5", 23deg, 2001).
V2252 Ori    VB B (A = NSV 16435, 11.05m; AB 7", 66deg, 2001).
V2254 Ori    Multiple.
V2255 Ori    Multiple (GCVS NAME FOR NSV 16443 11", 122deg, 2001; other components).
V2256 Ori    VB B (A = V1495 Ori, 12.24m; AB 9", 71deg, 2001).
V2257 Ori    VB C (A 11.05m, B 11.44m; AB 7", 66deg, AC 13", 137deg, 2001).
V2261 Ori    VB A (B = GCVS NAME FOR NEXT REMARK, 6", 17deg, 2001).
V2263 Ori    VB B (A = GCVS NAME FOR PREVIOUS REMARK; AB 6", 17deg, 2001).
V2266 Ori    Multiple (GCVS NAME FOR No. 8478 11", 302 deg, 2001; other components).
V2270 Ori    Multiple (NSV 16454 10.96m, 10", 65deg, 2001; other components).
V2271 Ori    VB (B = JW 474, 2.4", 24deg, 1961).
V2272 Ori    VB A (B 13.63m, 12", 331deg, 2001).
V2276 Ori    VB B (A 14.49m; AB 7", 173deg, 2001).
V2279 Ori    VB A (B = AC Ori 3" s).
V2280 Ori    VB A (B 12.57m, 5", 215deg, 2001).
V2283 Ori    VB B (A 13.00m; AB 9", 259deg, 2001).
V2284 Ori    Multiple.
V2288 Ori    Multiple.
V2291 Ori    VB A (B 13.47m, 7", 18deg, 2001).
V2292 Ori    Multiple (NSV 16466 12.56m, 12", 68:deg).
V2294 Ori    VB B (A 12.44m, 10", 59deg, 2001).
V2297 Ori    NSV 16469 9" nf.
V2299 Ori    VB A (B 4" s).
V2300 Ori    VB B (A = V1812 Ori, 10.60m; AB 9", 244deg, 2001).
V2301 Ori    VB C (A 8.76m, B = LZ Ori, 9.30m; AB 14", 220deg, AC 25", 226deg, 2001).
V2304 Ori    Multiple.
V2309 Ori    VB B (A 13.63m; AB 5", 300deg, 2001).
V2314 Ori    VB A (B 12.32m, 5", 16deg, 2001).
V2317 Ori    VB A (B 15.50m, 5", 300deg, 2001).
V2318 Ori    VB A (B 14.04m, 10", 69deg, 2001).
V2321 Ori    VB (2"). Multiple (V1336 Ori 5", 133deg, 1961; NSV 16467 10.10m, 10", 286deg, 2001; other components).
V2325 Ori    Multiple.
V2326 Ori    VB B (A 10.91m; AB 12", 115deg, 2001).
V2330 Ori    VB B (A 10.15m; AB 10", 69deg, 2001).
V2333 Ori    Multiple.
V2336 Ori    Multiple.
V2338 Ori    Multiple.
V2343 Ori    VB A (B = NSV 16486, 13.43:m, 9", 68deg, 2001).
V2346 Ori    VB B (A = GCVS NAME FOR NSV 16495; AB 10", 275deg, 2001).
V2350 Ori    V1516 Ori 11"nf.
V2352 Ori    VB B (A 13.65m; AB 6", 127deg, 2001).
V2353 Ori    Multiple.
V2354 Ori    VB A (B 6" sf).
V2355 Ori    VB B (A = GCVS NAME FOR NSV 2307; AB 13", 214deg, 2001; NSV 16490 close to A).
V2359 Ori    VB (0.8").
V2360 Ori    VB A (B = GCVS NAME FOR No. 9248, 10", 275deg, 2001; C 14.71m, 14", 240deg, 2001).
V2362 Ori    VB A (B 13.54m, 7", 83deg, 2001).
V2363 Ori    VB A (B = V1521 Ori; AB 7", 264deg, 2001).
V2364 Ori    VB A (B = GCVS NAME FOR No. 9305, 13", 214deg, 2001; NSV 16490 3" n).
V2366 Ori    VB B (A 12.01m; AB 11", 6deg, 2001).
V2372 Ori    VB A (B 10.98m, 8", 1deg, 2001).
V2373 Ori    VB B (A = V1521 Ori; AB 6", 90deg, 2001).
V2374 Ori    VB AB (0.7"). Multiple (NSV 16503 11.42mJ, 6", 330deg, 2001; other components).
V2377 Ori    VB B (A = NSV 16506, 13.64m; AB 4", 40deg, 1991).
V2378 Ori    VB B (A = AG Ori; AB 12", 185deg, 2001).
V2383 Ori    Multiple (V1524 Ori 9", 225deg, 2001; other components).
V2384 Ori    Min II = 14.81. MinII - MinI = 0.67P.
V2387 Ori    VB B (A 13.80m; AB 7", 78deg, 2001).
V2389 Ori    VB A (B 6" sf).
V2401 Ori    VB B (A 13.05m; AB 5", 321deg, 2001).
V2404 Ori    VB B (A = V561 Ori, 11.78m; AB 9", 250deg, 2001).
V2405 Ori    VB A (B 14.81m, 5", 285deg, 2001).
V2410 Ori    VB B (A = V1531 Ori; AB 7", 163deg, 2001).
V2413 Ori    VB A (B 3" f).
V2414 Ori    VB B (A = V1017 Ori; AB 10", 283deg, 2001).
V2415 Ori    VB B (A = NSV 16523 8" sp).
V2417 Ori    VB AB (1").
V2423 Ori    VB A (B = V1400 Ori, 6", 43deg, 2001).
V2425 Ori    Multiple (NSV 16535 12" nf; other components).
V2435 Ori    VB A (B 15.3m, 6", 138deg, 2001).
V2442 Ori    VB C (A 11.63m, B 11.70m; AB 3", 257deg, AC 10", 349deg, 2001).
V2444 Ori    VB A (B = GCVS NAME FOR NSV 16541, 6", 144deg, 2001).
V2448 Ori    VB B (A = GCVS NAME FROM PREVIOUS REMARK; AB 6", 144deg, 2001).
V2449 Ori    VB (AK Ori 9" s).
V2451 Ori    VB B (A 2.9mV, C = NSV 2342, 9.7mV; AB 11", 141deg, AC 49", 103deg, 2002).
V2454 Ori    VB A (B 10" np).
V2458 Ori    VB C (A = GCVS NAME FOR NEXT REMARK, B 11.34m; AB 9", 286deg, AC 6", 349deg, 2001).
V2460 Ori    VB A (B 11.34m, C = GCVS NAME FOR PREVIOUS REMARK; AB 9", 286deg, AC 6", 349deg, 2001).
V2464 Ori    VB B (A 11.29m; AB 11", 14deg, 2001).
V2467 Ori    VB B (A = NSV 02331, 11.77m, C 13.91:m; AB 7", 20deg, AC 11", 13deg, 2001).
V2476 Ori    VB A (B 13.70m, 11", 230deg, 2001).
V2479 Ori    VB B (A = V1549 Ori, AB 6", 117deg, 2001).
V2481 Ori    VB A (B 15.02m, 6", 13deg, C 16.39m, 10", 139deg, 2001).
V2483 Ori    VB A (B 14.76m, 9", 19deg, 2001).
V2484 Ori    VB A (B 12.38m, 7", 2deg, 2001).
V2491 Ori    VB A (B 13.12m, 6", 37deg, 2001).
V2492 Ori    VB B (A = GCVS NAME FOR NEXT REMARK; AB 8", 344deg, 2001).
V2494 Ori    VB A (B = GCVS NAME FOR PREVIOUS REMARK, 8", 344deg, 2001).
V2495 Ori    VB B (A = GCVS NAME FOR NSV 2341; AB 11", 342deg, 1961; also fainter components).
V2497 Ori    VB B (A = NSV 2340, 11.23m, C 13.82m; AB 8", 160deg, AC 7", 258deg, 2001).
V2499 Ori    VB A (B = GCVS NAME FOR No. 10729, 11", 342deg, 1961; also fainter components).
V2500 Ori    VB A (B 8" n).
V2509 Ori    NU Ori 20" np. VB A (B 12.36m, 8", 147deg, 2001).
V2514 Ori    VB B (A = V565 Ori, 10.17m; AB 9", 7deg, 2001).
V2516 Ori    The periodic variations were reported for the bright state (above 14m J).
V2521 Ori    VB B (A = V359 Ori, C 11.28; AB 10", 290deg; AC 14", 306deg, 2001).
V2537 Ori    VB A (B 14.35m, 7", 215deg, 2001).
V2543 Ori    VB B (A = AM Ori, AB 4", 330deg, 2001).
V2568 Ori    VB A (B 13.86m, 11", 168deg, 2001).
V2575 Ori    VB B (A 7.98m; AB 15", 232deg, 2001).
V2592 Ori    Min II = 8.20. MinII - MinI = 0.40P.
V2602 Ori    VB A (B 13.65m, 11", 63deg, 2001).
V2603 Ori    VB A (B 14.98m, 7", 282deg, 2001).
V2608 Ori    VB A (B 13.70m, 7", 350deg, 2001).
V2615 Ori    VB B (A = OV Ori, 11.51m; AB 7", 287deg, 2001).
V2620 Ori    VB B (A 10.34m; AB 12", 170deg, 2001).
V2630 Ori    VB A (B 15.27m, 8", 310deg, C 15.84m, 8", 144deg, 2001).
V2651 Ori    VB B (A = NSV 2412, 11.48:m; AB 9", 219deg, 2001).
V2655 Ori    VB B (A 12.56m; AB 10", 48deg, 2001).
V2677 Ori    VB A (B 13.80m, 10", 152deg, 2001).
V2678 Ori    Multiple.
V2679 Ori    VB B (A = NSV 2424, 11.01m; AB 14", 46deg, 2001).
V2689 Ori    Type from [034].
V2712 Ori    Min II = 12.7.
V2729 Ori    VB C (A 12.57m, B 16.17m; AB 16", 117deg, AC 18", 132deg, 1999).
V2735 Ori    Min II = 9.43.
V2743 Ori    Min II = 13.9.
V2749 Ori    SB2, Porb = 18.74d.
V2751 Ori    SB1.
V2752 Ori    Type from [034].
V2757 Ori    Min II = 10.12.
V2758 Ori    SB2, Porb = 4.99d.
V2759 Ori    Min II = 10.62.
V2762 Ori    Min II = 10.31.
V2766 Ori    Amplitude(Min II)=  0.7mag.
V2767 Ori    Min II = 13.2 :.
V2768 Ori    Amplitude(Min II)=  0.4mag.
V2769 Ori    Amplitude(Min II)=  0.4mag:.
V2772 Ori    Min II = 12.35.
V2776 Ori    VB A (B 16.9m R, 6", 31deg, 1999).
V2777 Ori    VB A (B 16.0m R, 9", 88deg, 1999).
V2778 Ori    Min II = 10.50:. MinII - MinI = 0.44P.
V2780 Ori    Min II = 12.12. VB A (B 5", 139deg, 1999).
V2783 Ori    Min II = 10.63. VB A (B 12.9m, 7", 25deg, 1999).
V2784 Ori    Min II = 13.7.
V2787 Ori    Min II = 10.28.
V2788 Ori    Min II = 10.82:.
V2789 Ori    Min II = 11.4.
V2790 Ori    Min II = 11.64.
V2793 Ori    Min II = 13.6.
alf   Ori    VB A (B 14.5m, 39.8", 110deg). Min = 2410600 + 2070d*E
alf   Ori    (1840 - 1929) [01012]. Since 1929 - see Table.
alf   Ori    The main variation is superimposed by the waves
alf   Ori    with P = 200 - 400d. Dust-gaseous shell (r = 50")
alf   Ori    [09529].
del   Ori    VB A (A 0.217", 144deg, 1980; B 14.0m, 33.1", 227deg;
del   Ori    C 6.84m, 53.5", 359deg). Orion Belt cluster member.
del   Ori    Min II 2.20.
del   Ori    Apsidal motion (P = 210 yr). Shape of the light curve
del   Ori    varies. The intrinsic brightness variability of the
del   Ori    components is possible.
eps   Ori    Orion Belt cluster member.
eta   Ori    VB Aab (AC 0.037", 111deg, 1979.0, P = 9.219 yr [09535];
eta   Ori    B 4.8m, 1.60", 76deg, 1976.0; C 9.4m, 115", 51deg). EA/DM.
eta   Ori    Min II 3.57. The range of combined light variation of the
eta   Ori    components AAb (SB 2, P = 7.989268d), AC, and B is given
eta   Ori    in the Table. Outside eclipses there are sinusoidal light
eta   Ori    variations of the system with A(V) = 0.05m due to
eta   Ori    pulsations of the component Ab [09535] with P = 0.30197d
eta   Ori    [09536] or 0.30145d [09537]. According to [08566] these
eta   Ori    variations were not observed between 1970 and 1976.
pi. 5 Ori    Min II 3.73. The period is improved using radial
pi. 5 Ori    velocities [04627].
psi   Ori    VB A (B 11.1m, 2.7", 323deg; C 13.88m, 83", 196deg).
psi   Ori    Min II 4.58. The period is determined on the base of
psi   Ori    radial velocities [09541].
R     Pav    Pvar. Max = 2411219 + 228.34d (JD2411000 - 18500);
R     Pav    Max = 2418527 + 230.95d*E (JD2418500 - 30000);
R     Pav    since JD2430000 - see Table.
S     Pav    P var. Max = 2421479 + 389.64d*E(JD2421000 - 31000);
S     Pav    since JD2431000 - see Table. Delta(m) var strongly.
S     Pav    Min II is sometimes observed after Max I.
T     Pav    P var. Max = 2413328 + 243.45d*E(JD2405700 -
T     Pav    25500); Max = 2425499 + 245.11d*E(JD2425500 -
T     Pav    32500); since JD2432500 - see Table.
V     Pav    VBA (B 14.0m vis, 15", 327deg). Mean brightness var,
V     Pav    P2 = 3735d, 9.7m - 10.7m.
W     Pav    P var. Before JD2431000 Max = 2413778 + 282.92d*E;
W     Pav    since JD2431000 - see Table.
RT    Pav    Mean light var, 10.4m - 11.1m  1649, P2 = 757d.
SU    Pav    P var. Max = 2430036 + 245.18d*E (JD2411000 - 30100)
SU    Pav    [00001]; during JD247700 - 40000 - see Table.
SX    Pav    mu alpha = +0.0166s, mu delta = -0.05".
TW    Pav    Before JD2420400 Max = 2417760 + 397.d*E.
YY    Pav    Delta(m) var strongly. P possibly is twice longer, in that
YY    Pav    case Min II 14.4.
AR    Pav    Depth of eclipses Delta(m) = 2m B, d = 0.05P. Expanding
AR    Pav    shell.
BD    Pav    Only one outburst was observed [00629]. Brightness
BD    Pav    flickering. Eclipses according to the elements
BD    Pav    Min I = 2444412.676 + 0.1793015d*E, Delta(m) ~0.5m [09191].
BD    Pav    Outside outburst, 15.40m - 16.21m.
BF    Pav    Min II 11.9.
BI    Pav    Min II (Delta(m) ~0.05m) is possible.
DF    Pav    Epoch of min is given. Light curve shape strongly var.
DN    Pav    Delta(S) = 8:.
DW    Pav    Min II 16.3.
EG    Pav    Twice shorter P is possible [00001].
EL    Pav    Min II 15.5.
EN    Pav    Elements need confirmation.
EQ    Pav    Red.
FY    Pav    Min II? JD2436784.37.
HL    Pav    Blazhko effect?
HP    Pav    Min II 15.5.
HQ    Pav    Min II 12.7.
HY    Pav    Min II 12.1.
IL    Pav    RRC type is possible.
KR    Pav    Min II 14.1.
KZ    Pav    VB A (B 8.7m, 6.7", 119deg, 1971; C 9.2m, BC 1.0", 329deg,
KZ    Pav    1971). P var. Min = 2430448.617 + 0.949880d*E
KZ    Pav    (JD2416000 - 30000) [00001]; since JD2430000 - see Table.
KZ    Pav    Min II is present.
LL    Pav    Min II 15.1.
LO    Pav    Min II 16.5.
LR    Pav    Min II 15.3.
LT    Pav    Min II 12.2.
LV    Pav    Min II 14.3.
LY    Pav    Min II 14.9.
MQ    Pav    Epoch of Min is given. EW/KW type with twice longer P is
MQ    Pav    possible.
MR    Pav    Possible elements Max = 2436731.40 + 0.3737d*E [00001].
MS    Pav    Min II 14.1.
MW    Pav    d = 0.08P. Min II 8.92, dII = 0.11P.
NP    Pav    Deep Min II.
NW    Pav    [A/H] = -0.7.
OY    Pav    The chart in [06286] is wrong.
V0382 Pav    Type EW: is also possible.
V0399 Pav    Symbiotic spectrum.
V0400 Pav    MinII 9.23.
V0413 Pav    P varies, dP/dt =+1.29 x 10^(-5) d/yr.
V0416 Pav    P0 is tabulated, P1 = 0.36574d.
kap   Pav    P var. Max = 2419619.38 + 9.0898d*E (JD2411930 - 22550);
kap   Pav    Max = 2425987.12 + 9.1028d*E (JD2422550 - 26980);
kap   Pav    Max = 2430530.67 + 9.0833d*E (JD2426980 - 31345);
kap   Pav    Max = 2433239.87 + 9.0956d*E (JD2431345 - 34045);
kap   Pav    Max = 2434693.11 + 9.0653d*E (JD2434045 - 37000);
kap   Pav    since JD2440000 - see Table. [Fe/H] = 0.0/ - 0.4.
kap   Pav    Moderately high Z coordinate (IZI ~240 pc provided
kap   Pav    the period - luminosity relation for DCEP stars is valid),
kap   Pav    low radial velocity. The period is not typical
kap   Pav    for CW stars. Ca II emission was noticed in the spectrum.
lam   Pav    VB A (B 12.4m, 63.1", 206deg).
rho   Pav    The main light variation P1 (see Table) with a
rho   Pav    semiamplitude delta(y) = 0.0069m is superposed by
rho   Pav    oscillations with P2 = 0.1131d (delta(y) = 0.0031m),
rho   Pav    P3 = 0.1612d (delta(y) = 0.0029m).
R     Peg    OH, H2O, SiO maser. P var. Max = 2396327 + 381.9d*E
R     Peg    (JD2396300 - 2408200); Max = 2413012 + 371.4d*E
R     Peg    (JD2413000 - 19800); Max = 2420092 + 379.77d*E
R     Peg    (JD2420000 - 31100) [00960]; since JD2431100 - see Table.
T     Peg    P var. Max = 2398452 + 371.0d*E (JD2398400 - 2408900);
T     Peg    Max = 2413697 + 386.8d*E (JD2413600 - 18700);
T     Peg    Max = 2421016 + 362.5d*E (JD2420900 - 28000) [00960];
T     Peg    Max = 2434343 + 376.0d*E (JD2428300 - 34300);
T     Peg    Max = 2440984 + 368.7d*E (JD2434300 - 41000);
T     Peg    since JD2441000 - see Table.
U     Peg    Min II 9.73. P var.
U     Peg    There is a square term in the elements:
U     Peg    -2.468D*10**(-11)*E**2.
U     Peg    0 - C = 0.00323d*sin((2pi/16330)E + 0.418pi). Shape of
U     Peg    the light curve varies.
W     Peg    SiO maser. P var. Max = 2413819 + 343.2d*E
W     Peg    (JD2413800 - 26600); Max = 2427162 + 345.5d*E
W     Peg    (JD2426600 - 32100) [00960]; Max = 2439690 + 348.75d*E
W     Peg    (JD2432300 - 39700) [00001]; since JD2441400 - see Table.
X     Peg    P var. Max = 2414713 + 200.3d*E (JD2414700 - 21300);
X     Peg    Max = 2420105 + 204.3d*E (JD2420100 - 23800);
X     Peg    Max = 2423570 + 199.8d*E (JD2423600 - 31000) [00960];
X     Peg    Max = 2432006 + 208d*E (JD2431000 - 32100);
X     Peg    Max = 2434206 + 200.0d*E (JD2432100 - 39300);
X     Peg    since JD2438400 - see Table.
Z     Peg    P var. Max = 2415433 + 318.9d*E (JD2398800 - 2420550);
Z     Peg    Max = 2420207 + 328.0d*E (JD2420200 - 32000) [00960];
Z     Peg    Max = 2432005 + 325.8d*E (JD2432000 - 37900);
Z     Peg    Max = 2437870 + 319d*E (JD2437500 - 40100);
Z     Peg    Max = 2442086 + 328.0d*E (JD2440100 - 43100);
Z     Peg    since JD2442100 - see Table.
RR    Peg    P var. Max = 2417582 + 268.3d*E (JD2416700 - 17850)
RR    Peg    [00001]; Max = 2417859 + 260.8d*E (JD2417850 - 21000)
RR    Peg    [00960]; since JD2421000 - see Table.
RS    Peg    P var. Max = 2415846 + 431.5d*E (JD2415800 - 18450);
RS    Peg    Max = 2418434 + 404.1d*E (JD2418400 - 24200);
RS    Peg    Max = 2424514 + 413.4d*E (JD2424500 - 34900) [00960];
RS    Peg    Max = 2436496 + 403.4d*E (JD2435700 - 38600) [00001];
RS    Peg    since JD2438500 - see Table.
RT    Peg    VB A (B 10.5m, 15.6", 291deg). P var.
RT    Peg    Max = 2423609 + 215.0d*E (JD2416000 - 24300);
RT    Peg    Max = 2428149 + 216.6d*E (JD2424300 - 32100);
RT    Peg    since JD2432100 - see Table.
RU    Peg    VB A (B 12.5m, 12", 18deg); SB2 (Porb = 0.3746d [09570]).
RU    Peg    There are also light oscillations with P = 11.6s
RU    Peg    and 50s [09571].
RV    Peg    Emission. Light curve (1907 - 1973) [09572]. P var.
RV    Peg    Max = 2428735 + 388.4d*E (JD2417000 - 32640);
RV    Peg    Max = 2430680 + 390.9d*E (JD2430200 - 38900);
RV    Peg    since JD2438800 - see Table.
RW    Peg    P var. Max = 2419393 + 208.4d*E (JD2412700 - 19400);
RW    Peg    Max = 2421520 + 213.0d*E (JD2419390 - 21550);
RW    Peg    Max = 2427133 + 208.0d*E (JD2421500 - 27150);
RW    Peg    since JD2427300 - see Table.
RX    Peg    P2 = 110d:.
RY    Peg    VB B (A = RZ Peg; B 20", 252deg).
RZ    Peg    VB A (B = RY Peg:20", 252deg). SC 6/9 - e. P var.
RZ    Peg    Max = 2423361 + 441.4d*E (JD2411400 - 26450);
RZ    Peg    Max = 2431215 + 434.0d*E (JD2426400 - 33000);
RZ    Peg    since JD2433000 - see Table.
SS    Peg    P var. Max = 2416390 + 410.8d*E (JD2415500 - 20000);
SS    Peg    Max = 2422235 + 423.8d*E (JD2420000 - 27000);
SS    Peg    Max = 2427270 + 403.4d*E (JD2427000 - 29000);
SS    Peg    Max = 2437218 + 416.35d*E (JD2428500 - 43000);
SS    Peg    since JD2443000 - see Table.
SV    Peg    H2O emission.
SX    Peg    S 2.5/6 e. P var. Max = 2436043 + 306.56d*E
SX    Peg    (JD2414800 - 38300); since JD2438300 - see Table.
TU    Peg    P var. Max = 2417800 + 320.8d*E (JD2404300 - 18450);
TU    Peg    Max = 2420730 + 328.4d*E (JD2418450 - 20800);
TU    Peg    Max = 2428080 + 319.6d*E (JD2420800 - 31600);
TU    Peg    since JD2432800 - see Table.
TW    Peg    H2O maser. The basic light variation with the period given
TW    Peg    in the Table is superimposed by small oscillations
TW    Peg    with P = 94.13d.
TY    Peg    Min II 10.2. P var. Min I hel = 2419520.476 +
TY    Peg    3.0922754d*E (JD2412300 - 19600) [02389]; Min I hel =
TY    Peg    2425918.348 + 3.092252d*E (JD2419600 - 26000)
TY    Peg    [00001]; since JD2426000 - see Table.
TZ    Peg    P var? Max = 2425892 + 213.7d*E (JD2410000 - 28000);
TZ    Peg    since JD2430000 - see Table.
UU    Peg    OH, H2O maser.
UW    Peg    According to [08837] P = 60d.
UX    Peg    P var. Min = 2428428.386 + 1.544618d*E (JD2422100 -
UX    Peg    28430) [00230]; Min = 2431273.597 + 1.544632d*E
UX    Peg    (JD2428420 - 34000) [00001]; since JD2434000 - see Table.
VV    Peg    Delta(S) = 8. P var. Max = 2420105.296 + 0.48837765d*E
VV    Peg    (JD2420000 - 28900); Max = 2433217.268 + 0.48838307d*E
VV    Peg    (JD2432800 - 38000) [03506]; since JD2438000 - see Table.
VW    Peg    P = 2.341295d?
VX    Peg    The basic light variation is superimposed by the secondary
VX    Peg    one with P = 80 - 90d:.
VZ    Peg    [Fe/H] = -1.75.
WW    Peg    P var. Max = 2433142 + 371.6d*E (JD2415670 - 33200)
WW    Peg    [00001]; since JD2436800 - see Table.
ZZ    Peg    Min II 12.5.
AE    Peg    P var. Max = 2415470.866 + 0.4967388d*E (JD2415500 -
AE    Peg    21000); Max = 2426161.544 + 0.496725d*E (JD2425400 -
AE    Peg    31500); Max = 2432632.809 + 0.496692d*E (JD2431500 -
AE    Peg    36000) [00001]; during JD2436000 - 40000 - see Table.
AE    Peg    Delta(S) = 6.3.
AG    Peg    SB2 (Porb = 820d [09580]).
AG    Peg    Maximum of brightness was in 1870, then the very
AG    Peg    slow light decrease was observed that was superimposed
AG    Peg    since 1935 by periodical light oscillations with
AG    Peg    A = 0.4m V
AG    Peg    and P = Porb: Min = 2428250 + 827.d*E ( JD2428000-43000)
AG    Peg    [09587]. After JD2442300 the period probably has changed:
AG    Peg    Min = 2442370 + 760d*E [09587]. In 1962 - 1979 the range of
AG    Peg    brightness was 7.95m - 8.55m V; M - m = 0.50P.
AG    Peg    Light minima correspond to the epochs of inferior
AG    Peg    conjunction of M 3 III component. Spectrum var: Beq
AG    Peg    (1893 - 1919); since 1922 the spectrum is symbiotic one,
AG    Peg    the M star spectrum being more noticeable.
AG    Peg    Surrounded by a radio nebula with 1" half-power diameter.
AN    Peg    P var. Max = 2428045 + 274.1d*E (JD2424500 - 38500)
AN    Peg    [09581]; since JD2438500 - see Table.
AO    Peg    Delta(S) = 4.3.
AQ    Peg    Min II 10.47; d = 0.030P. P var. Min I = 2424749.335 +
AQ    Peg    5.548419d*E (JD2424000 - 34000) [00980];
AQ    Peg    since JD2434000 - see Table.
AS    Peg    Of the two stars circled in the chart in [06286], the southern
AS    Peg    component varies.
AT    Peg    Min II 9.04. P var. Min I = 2425862.337 + 1.1460988d*E
AT    Peg    (JD2425800 - 37500) [00001]; Min I = 2437497.542 +
AT    Peg    1.146080d*E (JD2437490 - 40000) [06101]; Min I =
AT    Peg    2440407*4370 + 1.1461007d*E (JD2440000 - 42400)
AT    Peg    [00001]; since JD2442400 - see Table.
AU    Peg    Cepheid in a close binary system.
AU    Peg    SB1 (Porb = 53.319d, K1 = 41.8 km/s, gamma = -4.1 km/s,
AU    Peg    E = 0.12 [09582]). [Fe/H] = 0.1.
AU    Peg    P var. Max = 2428729.76 + 2.3978d*E (JD2426500 - 28750)
AU    Peg    [00916]; Max = 2433151.976 + 2.38934d*E (JD2433150 - 35800);
AU    Peg    Max = 2439039.08 + 2.39079d*E (JD2435800 - 39100) [00001];
AU    Peg    since JD2441700 - see Table.
AU    Peg    There is a square term in the elements given in the Table:
AU    Peg    +2.246d*10**(-6)*E**2. The shape of the light curve varies:
AU    Peg    0.20P <  M - m < 0.47P.
AV    Peg    P var. Max = 2416347.713 + 0.39036510d*E
AV    Peg    (JD2414000 - 26500) [00752]; Max = 2426582.301 +
AV    Peg    0.39037015d*E (JD2426500 - 36000) [09584];
AV    Peg    since JD2436000 - see Table. [Fe/H] = +0.02.
AW    Peg    d = 0.07P, Min II 7.60.
BB    Peg    Depth of Min II 0.60m.
BB    Peg    There is a square term in the elements given in the Table:
BB    Peg    +2.3d*10**(-11)*E**2. dI = 0.05P; dII = 0.00P.
BF    Peg    P var. Max = 2426589.293 + 0.495796d*E + 2.8d*10**(-9)*E**2
BF    Peg    (JD2426500 - 28800) [00522]; Max = 2433200.312 +
BF    Peg    0.495796d*E (JD2429400 - 33200) [00001]; Max =
BF    Peg    2437583.343 + 0.495674d*E (JD2437500 - 39400)
BF    Peg    [00001]; since JD2442650 - see Table.
BG    Peg    P var. Min = 2427386.3705 + 1.952452d*E (JD2426000 - 35000)
BG    Peg    [03567]; Min = 2436453.509 + 1.95238d*E (JD2435000 - 43500)
BG    Peg    [03624]; since JD2443500 - see Table.
BH    Peg    P var. Max = 2426596.535 + 0.64101381d*E
BH    Peg    (JD2426500 - 28200) [01038]; since JD2434400 - see Table.
BH    Peg    Blazhko effect. A var.
BH    Peg    Max (O - C) = 2442929.03 + 39.8d*N [09588]. (k - b)2 = 0.09;
BH    Peg    Delta(S) = 5.
BI    Peg    Waves with a cycle of 60 - 80d are superimposed.
BK    Peg    Min II 10.47.
BO    Peg    Min II 11.6. P var. Min I = 2427655.460 + 0.5804342d*E
BO    Peg    (JD2426500 - 35100) [02263]; since JD2444000 - see Table.
BP    Peg    P1 = 0.084510d; P1:P0 = 0.77. Beat
BP    Peg    period Pb = 0.3698d [06604].
BS    Peg    The chart in [06286] is wrong.
BU    Peg    Observations are represented by the elements in the
BU    Peg    intervals JD2432000 - 34000, JD2438200 - 41400.
BX    Peg    Depth of Min II 0.62m; dI = 0.05P; dII = 0.00P.
BX    Peg    P var. Min I = 2431323.278 + 0.2804238d*E
BX    Peg    (JD2424700 - 39000) [00279]; since JD2439000 - see Table.
BY    Peg    P var. Min I = 2424745.75 + 0.34193403d*E
BY    Peg    (JD2424700 - 35400); since JD2435000 - see Table.
CC    Peg    Min II 12.9.
CG    Peg    Delta(S) = 2. P var?
CU    Peg    d = 0.010P. P var. Min = 2433895.463 + 3.8801345d*E
CU    Peg    (JD2425500 - 34000) [00001]; Min = 2434221.392 +
CU    Peg    3.880196d*E (JD2434000 - 36500) [07929];
CU    Peg    since JD2436500 - see Table.
CZ    Peg    Min II 13.9.
DF    Peg    Min II 9.2.
DG    Peg    P var. Max = 2425857 + 148.15d*E (JD2425500 -
DG    Peg    33500); since JD2433500 - see Table.
DH    Peg    P var. Max = 2414981.537 + 0.25550478d*E
DH    Peg    (JD2414000 - 24000) [01158];
DH    Peg    Max = 2427695.390 + 0.2555107d*E (JD2424000 - 33500)
DH    Peg    [09590]; since JD2433500 - see Table. [Fe/H] = -0.9.
DI    Peg    Min II 9.59. P var. Min I = 2425644.315 + 0.7118144d*E
DI    Peg    (JD2425500 - 30000) [02431]; Min I = 2437559.4096 +
DI    Peg    0.7118182d*E (JD2430000 - 40000) [09592]; Min I =
DI    Peg    2440159.6796 + 0.71181417d*E (JD2440000 - 44500);
DI    Peg    since JD2444500 - see Table.
DK    Peg    d = 0.04P. P var. Min = 2427745.388 + 1.631801d*E
DK    Peg    (JD2427700 - 33700); since JD2433700 - see Table.
DM    Peg    d = 0.03P; Min II 11.0.
DN    Peg    Mean brightness varies with cycles 800 - 1400d and
DN    Peg    A = 0.2m - 0.4m.
DO    Peg    P var. Min = 2434272.350 + 2.61394d*E (JD2428000 - 34700)
DO    Peg    [00485]; since JD2434700 - see Table.
DV    Peg    Min II 12.1.
DY    Peg    P var. Max = 2432751.9624 + 0.072926372d*E
DY    Peg    (JD2429000 - 38000); since JD2438000 - see Table.
DY    Peg    The basic pulsation is superimposed by the secondary one
DY    Peg    with P1 = 0.05570d [09594]. A var, M - m var (Pi = 0.2358d):
DY    Peg    0.55m < A < 0.67m, 0.24P < M - m < 0.42P. Delta(S) = 6.
DZ    Peg    P var. Max = 2429127.211 + 0.6073407d*E
DZ    Peg    (JD2419000 - 28800); Max = 2429127.189 + 0.6073761d*E
DZ    Peg    (JD2429100 - 33500); since JD2433500 - see Table.
EE    Peg    Min II 7.06. The third body (Porb = 1464d, T0 = 2443120).
EF    Peg    VB B (A 14.0m; B 5", 305deg).
EH    Peg    d = 0.08P.
EQ    PegA   VB A (B = EQb Peg; A = 6.87", Porb = 359 yr, E = 0.20.
EQ    PegA   [09597]); mu = 0.560", P = 91.7deg. A (B) >= 1.4m.
EQ    PegB   VB B (A = EQa Peg). a = 6.87'' P orb = 1464d,
EQ    PegB   T0 = 2443120. A(U) >= 1.9m.
ET    Peg    Delta(S) = 4.
EU    Peg    Min II 12.3.
EZ    Peg    On 1943 November 16 the spectrum of the star was B [02875];
EZ    Peg    probably at that time the star had a flare.
FL    Peg    Min II 14.0.
FU    Peg    Blazhko effect (Pi = 150d); A var;
FU    Peg    15.2m <= Max <= 15.8m; 0.15P <= M - m <= 0.50P.
GH    Peg    Depth of Min II 0.13m.
GR    Peg    P var. Max = 2436492 + 69.93d*E (JD2436420 - 38740);
GR    Peg    since JD2440470 - see Table.
GT    Peg    mu = 0.51", P = 96deg. Epoch of the light minimum is given.
GT    Peg    During the flares A(U) < 3.6m.
GV    Peg    Delta(S) = 5:.
GW    Peg    Min II 15.1.
GX    Peg    SB1 (Porb = 2.340939d [06103]).
GZ    Peg    VB A (B 10.6m, A3V, 32.7", 198deg).
HN    Peg    [Fe/H] = -0.09. Epoch of light minimum is given.
HN    Peg    The variability of emission in H and K call lines with
HN    Peg    P = 4.63d was detected [09600].
HP    Peg    Vr = -381 km/s.
HR    Peg    S4+/1+ .
HZ    Peg    Min II 17.6.
II    Peg    mu = 0.575", p = 86.5deg. SB1
II    Peg    (T0 = 2443030.396 + 6.724464d*E); T0 is the epoch of the
II    Peg    inferior conjunction of K-star. The epoch of the
II    Peg    distortion wave maximum is given in the Table. Mean
II    Peg    brightness of the system varies.
IK    Peg    SB1 (Porb = 21.724d). Multiperiodicity [09609].
IM    Peg    SB1 (Porb = 24.649d).
QQ    Peg    Variability needs confirmation.
V0341 Peg    SB, Porb = 2.1779d.
V0342 Peg    Suspected SB.
V0405 Peg    Type ZAND is also possible.
V0407 Peg    MinII 9.69. O'Connell effect.
V0415 Peg    VB (8.9m, 9.1m, 0.2", 316deg, 1996).
V0416 Peg    VB (8.1m, 10.0m, 4", 36deg, 1991).
V0418 Peg    SB2, Porb = 135.19d.
V0421 Peg    Min II = 8.63.
V0429 Peg    Blazhko effect, P = 80.2d.
V0443 Peg    Blazhko effect from Catalina data [001].
V0444 Peg    Superhumps: P = 0.097762d [233].
V0460 Peg    The period of ellipsoidal variations is tabulated. Pulsational periods: 0.06479d and 0.06337d. The A8 component pulsates.
V0473 Peg    O'Connell effect.
V0479 Peg    Period varies.
V0492 Peg    P = 0.11068d for the main DSCTC mode. Multiperiodic, several other GDOR and DSCTC periods.
V0499 Peg    VB A (A 10.90mJ; B 11.50mJ, 9", 324deg, 2000).
V0510 Peg    Multiperiodic.
V0513 Peg    Porb = 0.17918d.
V0517 Peg    Blazhko effect?
V0521 Peg    Porb = 0.05986d.
V0533 Peg    VB AB (A 9.7mJ; B 11.3mJ, 4", 1 deg, 1998).
V0537 Peg    Porb = 0.42234d.
V0550 Peg    Blazhko effect.
V0553 Peg    Blazhko effect?
V0585 Peg    Multiperiodic.
V0598 Peg    Porb is tabulated. Pspin = 0.02893d.
V0615 Peg    Porb = 0.240946d from spectroscopy.
bet   Peg    VB A (B 11.2m, 109", 211deg).
eps   Peg    VB A (B 12.66m, 81", 325deg; C 8.65m, 140", 321deg).
eps   Peg    Usually varies in the range 2.29m - 2.44m V. On 1972
eps   Peg    september 26/27 in the interval 23h58m - 00h02m UT it was
eps   Peg    bright (0.7m V), then at 00h09m UT decreased to 2.4m V
eps   Peg    [06875]. On 1847 November 5 the star was 3.5m, then the
eps   Peg    brightness increased but on November 6 it was still
eps   Peg    fainter than normal [09606].
tau   Peg    P2 = 0.04895d; PB = 0.4943d.
S     Per    In the region of the open cluster h, khi Per.
S     Per    OH, H2O, SiO maser.
S     Per    In 1920 - 1969 there were secondary
S     Per    waves with cycles of 300d - 700d and Delta(m) ~1m [08630];
S     Per    in 1935 - 1961 P1 = 807d, P2 = 930d [09694].
T     Per    Other periodicities were noted. In the region
T     Per    of open cluster h, khi Per.
U     Per    P var. Max = 2411683 + 316.10d*E (before JD2422500);
U     Per    Max = 2422748 + 326.53d*E (JD2422500 - 34000);
U     Per    since JD2434000 - see Table.
V     Per    VB A (B 14m, 28", 278deg).
W     Per    P2 = 2667d +- 460d is superimposed.
X     Per    3U 0352 + 30. LX/Lopt = 10**(-2). ADS 2859 A (B =
X     Per    V397 Per, M3III, 22.5", 12deg). SB.
X     Per    IR excess. X-ray pulsar (P = 13.93m).
X     Per    Further periodicities were noticed in X-ray, optical,
X     Per    spectroscopic observations: 22.4h, 308.33d, 580.7d.
Y     Per    P var. Max = 2414990 + 254.74d*E (JD2415000 - 18000);
Y     Per    Max = 2418049 + 246.25d*E (JD2418000 - 22000);
Y     Per    Max = 2422242 + 253.62d*E (JD2422000 - 41000);
Y     Per    since JD2441000 - see Table.
Z     Per    d = 0.028P; Min II 9.8.
Z     Per    P var. Min = 2418173.663 + 3.056422d*E (JD2415000 -
Z     Per    19000) [01961]; Min = 2425481.416 + 3.05636d*E
Z     Per    (JD2419000 - 31000) [00978]; since JD2431000 - see Table.
RR    Per    P var. Max = 2424280 + 392.01d*E (JD2416000 - 28500);
RR    Per    since JD2428500 - see Table.
RS    Per    In the region of the open cluster h, khi Per.
RS    Per    According to [01053], P = 152d.
RT    Per    Min II 10.67. P var. Min = 2411963.2995 + 0.84941322d*E
RT    Per    (JD2411317 - 19400); Min = 2419702.3124 + 0.84940248d*E
RT    Per    (JD2419400 - 29300); Min = 2429751.6066 + 0.84941274d*E
RT    Per    (JD2429300 - 33000); since JD2433000 - see Table.
RV    Per    Min II 10.4. P var. Min = 2417972.345 + 1.973489d*E
RV    Per    (JD2417000 - 25500); since JD2432500 - see Table.
RW    Per    The light curve shape var,
RW    Per    d = 0.03P - 0.000P. Min II 9.78. P var. Before
RW    Per    JD2425720 Min = 2425720.0185 + 13.198910d*E;
RW    Per    Min = 2429217.5946 + 13.198399d*E (JD2425720 - 36700);
RW    Per    since JD2436700 - see Table.
RY    Per    d = 0.014P; Min II 8.65.
RZ    Per    S 3/7 e. P var. Before JD2430500 Max = 2415034 + 353.19d*E;
RZ    Per    since JD2430500 - see Table.
ST    Per    VB A (B 12.1m, 11.6", 6deg, 1928). d = 0.014P, Min II 9.62.
ST    Per    P var. Min = 2419030.5038 + 2.6483615d*E
ST    Per    (JD2418500 - 27000) [09740]; Min = 2429528.5897 +
ST    Per    2.6483488d*E (JD2427000 - 34600) [02389]; Min =
ST    Per    2439091.716 + 2.648353d*E (JD2439000 - 42400);
ST    Per    since JD2442400 - see Table.
SU    Per    In the region of the open cluster h, khi Per.
SV    Per    [A/H] = 0.6. SB2, hot companion.
SV    Per    P var? Before JD2435000 Max = 2419055.145 +
SV    Per    11.12875d*E [02431]; since JD2435000 - see Table.
SX    Per    [A/H] = 0. The chart in [08300]
SY    Per    In the region of the open cluster NGC 1528.
TU    Per    Delta(m), P var. Before JD2427200 Max = 2418572.288 +
TU    Per    0.6070775d*E; Max = 2427119.334 + 0.6070643d*E
TU    Per    (JD2427200 - 36000); since JD2436000 - see Table.
TV    Per    P2 = 1080d is superimposed.
TX    Per    [Fe/H] = -0.88. OH maser.
TZ    Per    VB A (B14m, 13", 290deg). Mu alpha = +0.012",
TZ    Per    mu delta = -0.050". In the region of the open
TZ    Per    cluster h, khi Per.
UX    Per    [A/H] = -0.3.
UY    Per    [A/H] = -0.3. In the region of the open clusters King 4,
UY    Per    Czernik 8.
UZ    Per    P2 = 91d is superimposed.
VV    Per    Twice shorter P is possible [00960].
VX    Per    In the region of the open cluster h, khi Per.
VX    Per    [A/H] = -0.2. P var. Since JD2431000 - see Table.
VY    Per    In the region of the open cluster h, khi Per.
VY    Per    [A/H] = -0.3.
VZ    Per    VB A (B 16.9m pg, 17", 180deg). In the region of the open
VZ    Per    cluster Tr 2.
WY    Per    P var. Min = 2425234.460 + 3.327126d*E (JD2421500 - 26000)
WY    Per    [01072]; since JD2441500 - see Table.
XX    Per    VB A (B 9.7m vis, 21", 176deg, 1909).
XX    Per    Mean brightness var, P = 4100d.
XY    Per    ADS 2788 AB (delta(mV) = 0.6m - 2.5m, 1.4", 75deg,
XY    Per    SpA = A2II, SpB = B6e). IR excess.
XZ    Per    Min II 11.6. P var? Min = 2425150.439 + 1.1516282d*E
XZ    Per    (JD2425000 - 29000) [00522]; Min = 2437932.411 +
XZ    Per    1.1516347d*E + 0.005d*sin(0.09091deg*E) (JD2432000 -
XZ    Per    38000) [00001]; since JD2438000 - see Table.
YZ    Per    In the region of the open cluster h, khi Per.
ZZ    Per    The coordinates are possibly erroneous.
AB    Per    d = 0.045P; Min II 10.5. VB (Delta(m) = 0.0m vis, 0.20",
AB    Per    86.4deg, 1978).
AD    Per    Mean brightness var, P = 2950d.
AD    Per    In the region of the open cluster h, khi Per.
AE    Per    P2 = 2150d is superimposed.
AG    Per    ADS 2990 A (B Delta(m) = 2.0m, 0.9", 225deg, 1975; C 12.6m,
AG    Per    36", 118deg, 1948). The combined brightness AB is given.
AG    Per    Min II 7.00, DII = 0.10P, dII = 0. Apsidal motion:
AG    Per    Min II - Min I = 1.01435d + 0.0884d*sin(0.0278deg*E +
AG    Per    49.1deg).
AR    Per    P var, nonlinear term: +1.18d*10**(-11)*E**2.
AR    Per    [Fe/H] = -0.17.
AS    Per    Delta(m) var, d (Delta(B))/dt = -0.01m/yr.
AV    Per    P = 250 - 300d.
AW    Per    SB2, companion B6V, Delta(m) (companion - AW) = 2.8m vis.
AX    Per    Epoch of Min is given. The variability with Delta(m) up to
AX    Per    0.7m pg is caused probably by the orbital motion. Outburst
AX    Per    activity is superimposed.
AY    Per    d = 0.009P.
BE    Per    In the region of the open cluster CR 39.
BI    Per    In the region of the open cluster Berk 9.
BL    Per    P = 125 - 130d.
BM    Per    [Fe/H] = -0.04.
BP    Per    Min II = Min I. In the region of the open cluster
BP    Per    Cr 39.
BU    Per    Max brightness var, P = 8.1yr [01085]. In the region of
BU    Per    the open cluster h, khi Per.
CC    Per    Min II 14.1.
CI    Per    P var (3.35d - 3.40d), possibly with a period of 4000d.
CI    Per    The light curve shape var.
CK    Per    d = 0.05P:.
CM    Per    d = 0.052P. In the region of the open cluster Stock 2.
CO    Per    In the region of the open cluster Stock 2.
CR    Per    Elements need confirmation. In the region of the open
CR    Per    cluster Stock 2.
CS    Per    In the region of the open cluster Stock 2.
CZ    Per    In the region of the open cluster h, khi Per.
DE    Per    d = 0.01P?
DF    Per    In the region of the open cluster h, khi Per.
DG    Per    d = 0.021P.
DK    Per    The depth of Min II 0.05m. In the region of the open
DK    Per    cluster h, khi Per.
DM    Per    Min II 8.02, DII = 0.17P.
DM    Per    Depths of Minima, the shape of Min II var.
DM    Per    In the region of the open cluster h, khi Per.
DO    Per    In the region of the open cluster h, khi Per.
DP    Per    In the region of the open cluster h, khi Per.
DR    Per    In the region of the open cluster h, khi Per.
DS    Per    In the region of the open cluster h, khi Per.
DT    Per    In the region of the open cluster h, khi Per.
DU    Per    In the region of the open cluster h, khi Per.
DV    Per    Min II 14.5.
DY    Per    In the region of the open cluster Tr 2.
DZ    Per    Min II 14.7. In the region of the open cluster Tr 2.
EL    Per    Before JD2428900 Max = 2427980 + 167d*E;
EL    Per    during JD2428900 - 31000 - see Table.
EO    Per    IR excess?
ER    Per    Mean brightness var, P ~900d.
EU    Per    Min brightness var, P ~900d.
EW    Per    Superimposed waves 70d - 180d.
EW    Per    In the region of the open cluster Stock 4.
EX    Per    Min II 12.5.
FM    Per    VB A (B 12.1m, 3", 285deg). P var? Max = 2429982.268 +
FM    Per    0.489199d*E (JD2428000 - 30600);
FM    Per    During JD2433700 - 36000 - see Table.
FR    Per    In the region of the open cluster NGC 1528.
FV    Per    Cycles 300 - 350d, 1800d:.
FX    Per    d = 0.04P. In the region of the open cluster NGC 1582.
FY    Per    Possible periods 0.0702d, 0.4407d.
FY    Per    Photometric spectral type B1V.
FZ    Per    In the region of the open cluster h, khi Per.
GH    Per    P = 220d is possible.
GK    Per    SB2 (sdBE + K2IVp).
GK    Per    The following types of activity are being observed after
GK    Per    the return to the normal brightness: rapid irregular
GK    Per    variations (Delta(m) ~0.1m in several minutes); irregular
GK    Per    fluctuations from night to night (Delta(m) up to 0.3m);
GK    Per    slow irregular variations (Delta(m) = 1.5m in several
GK    Per    dozen days); bursts with light increase in 10d - 30d and
GK    Per    decrease in 10d - 40d, Delta(m) up to 3.5m, the mean
GK    Per    interval between bursts being delta(t) = 820d [09686, 09788].
GK    Per    According to [10198], the radial velocities are
GK    Per    represented with the elements Max (Vr > 0) = 2444912.966 +
GK    Per    1.996803d*E (Kabs = 124 km/s, Kem = 34 km/s). According
GK    Per    to [10199], the 2d variation is modulated with a period
GK    Per    of 0.131623d, Max (delta(Vr)) ~2443787.995 (Kabs =
GK    Per    15 km/s, Kem = 20 km/s). During a burst the sinusoidal
GK    Per    modulation of X-ray flux was recorded,
GK    Per    Tmax = 24455555.67456 + 0.004066443d*E [09786].
GK    Per    ExpAnding envelope (0.454"/yr, 1948 - 1964;
GK    Per    0.432"/yr, 1964 - 1981, [09787]).
GP    Per    [A/H] = -0.5.
GQ    Per    According to [00021], Sp K0.
HQ    Per    [A/H] = -0.3.
HS    Per    In the region of the open cluster Stock 4.
HV    Per    d ~0.03P.
HW    Per    Min II 13.3. Min II - Min I = 0.45P:.
HY    Per    Three of the four min in [01079] are not satisfied with the
HY    Per    elements.
HZ    Per    [A/H] = -0.8. B_V: +1.93, +2.34.
II    Per    Min II 13.6. In the region of the open cluster NGC 1582.
IK    Per    Min II 11.6.
IM    Per    Min II 12.7. The elements need confirmation. In the region
IM    Per    of the open cluster Cr 39.
IO    Per    H2O maser.
IP    Per    IR excess.
IQ    Per    dI = 0.02P. Min II 7.88, DII = 0.12P, dII = 0.03P,
IQ    Per    Min II - Min I = 0.53P. P var? VB A (B = BD + 47deg 921,
IQ    Per    9.30m, A0V np:, 39.3", 175deg); SB1.
IT    Per    dI = 0.06P. Min II 10.0, DII = 0.24P:, dII = 0.16P:.
IT    Per    VB (Delta(m) = 1.7m, 12", 37deg).
IT    Per    The range of the combined brightness is given.
IW    Per    SB1. Min II 5.83.
IX    Per    The depth of Min II 0.02m.
IX    Per    VB A (B 10.6m, 5", 208deg).
IZ    Per    Min II 8.3.
KK    Per    In the region of the open cluster h, khi Per.
KP    Per    Beat phenomenon: P1 - see Table,
KP    Per    A1 = 0.0323m B; P2 = 0.1980855d, A2 = 0.0235M B; P3 =
KP    Per    0.2270986d, A3 = 0.0072M B.
KR    Per    Min II 11.1.
KS    Per    SB (Porb = 360.47d).
KS    Per    The main component is a helium star. Besides the
KS    Per    semiregular variability (see Table), variations were noted
KS    Per    with P = 50 - 100 Min and Delta(m) of several hundredths
KS    Per    of a magnitude. IR excess. Variable polarization (P - 1%).
KT    Per    Quasi-periodic oscillations during outbursts: P =
KT    Per    22.9s - 29.5s [05959], 82s, 90s, 147s [09791], Delta(m)
KT    Per    up to ~0.01m.
KV    Per    [Fe/H] = -0.96. P var. Max = 2428950.400 + 0.24942d*E
KV    Per    (JD2428950 - 29200); since JD2429500 - see Table.
KW    Per    Min II 10.8. P var. Min = 2426295.450 + 0.931255d*E
KW    Per    (JD2423400 - 39500) [04009]; since JD2440000 - see Table.
KY    Per    In the region of the open cluster h, khi Per.
KZ    Per    In the region of the open cluster h, khi Per.
LL    Per    In the region of the open cluster h, khi Per.
LM    Per    In the region of the open cluster h, khi Per.
LN    Per    In the region of the open cluster h, khi Per.
LO    Per    In the region of the open cluster h, khi Per.
LP    Per    In the region of the open cluster h, khi Per.
LQ    Per    In the region of the open cluster h, khi Per.
LR    Per    Very red. In the region of the open cluster h, khi Per.
LX    Per    mu alpha = +0.0065s, mu delta = -0.063". Min II 8.38m.
LX    Per    DII = 0.05P. Migrating distortion wave:
LX    Per    P = 475d [09792], Delta(m) up to 0.04m.
MS    Per    Min II 12.1.
MX    Per    IR excess.
NP    Per    Min II 13.0.
NR    Per    P var. Max = 2416780 + 323.0d*E (JD2415750 - 24550);
NR    Per    Max = 2435060 + 340.2d*E (JD243350 - 35400);
NR    Per    since JD2436700 - see Table.
NU    Per    A close pair, var is the southern star.
OV    Per    D ~2h.
PP    Per    In the region of the open cluster h, khi Per.
PR    Per    In the region of the open cluster h, khi Per.
QR    Per    Red.
QU    Per    d = 0.03P.
QW    Per    Min II 14.7:.
QX    Per    Min II 16.1.
V0345 Per    In the nebula NGC 1579.
V0346 Per    In the nebula NGC 1579.
V0347 Per    In the nebula NGC 1579.
V0351 Per    In the region of the open cluster h, khi Per.
V0352 Per    In the region of the open cluster h, khi Per.
V0354 Per    In the region of the open cluster h, khi Per.
V0355 Per    In the region of the open cluster h, khi Per.
V0356 Per    In the region of the open cluster h, khi Per.
V0357 Per    In the region of the open cluster h, khi Per. P = 0.21955d
V0357 Per    is possible.
V0358 Per    In the region of the open cluster h, khi Per.
V0359 Per    In the region of the open cluster h, khi Per.
V0360 Per    In the region of the open cluster h, khi Per.
V0360 Per    Other possible periods: 0.40036d, 0.40154d.
V0361 Per    In the region of the open cluster h, khi Per.
V0363 Per    Red.
V0364 Per    Min II 15.6, Max II 14.8.
V0365 Per    Min II 14.3:.
V0376 Per    P2 = 0.09165d, A2 = 0.016m; P1 - see Table,
V0376 Per    A1 = 0.037m. A var.
V0380 Per    SB (Porb = 26d?). The epoch of Min light is given.
V0382 Per    In the region of the open cluster h, khi Per.
V0392 Per    The southern component of a very close pair.
V0394 Per    H2O maser.
V0395 Per    VB A (B 3.5", 90deg).
V0396 Per    In the region of the open cluster alpha Per.
V0396 Per    Observations are also satisfied by P ~1.678d. According
V0396 Per    to [07586], P = 2.4928d or 1.6857d.
V0397 Per    ADS 2859 B (A = X Per; B 22.5", 12deg).
V0398 Per    IN type is also possible.
V0403 Per    In the region of the open cluster h, khi Per.
V0409 Per    Epoch of Min is given.
V0423 Per    ADS 2433 A (B 11.9m, 30.8", 99.2deg); SB.
V0423 Per    Porb is given.
V0424 Per    In the region of the open cluster h, khi Per. IR excess.
V0425 Per    VB A(B 12.8m, 3.6", C 14.3m, 6.8"). In the region of
V0425 Per    the open cluster h, khi Per.
V0428 Per    According to [08639], type IS?
V0432 Per    Min II 11.6.
V0434 Per    Min II 14.9.
V0436 Per    Min II 5.74; Min II - Min I = 0.413P; D II = 0.03P.
V0437 Per    In the region of the open cluster NGC 744.
V0438 Per    In the region of the open cluster h, khi Per. VB (8.7m,
V0438 Per    10.9m, 1".2, 26deg).
V0438 Per    Min II 8.34. The range of combined brightness
V0438 Per    variation is given. The bright component is
V0438 Per    considered to be variable. This suggestion
V0438 Per    needs verification.
V0439 Per    In the region of the open cluster h, khi Per.
V0440 Per    In the region of the open cluster h, khi Per. ADS 1820
V0440 Per    A (B 14.5m, 8".3, 122deg).
V0449 Per    Min II 13.3.
V0451 Per    Min II 15.8.
V0459 Per    In the alpha Per cluster.
V0461 Per    In the alpha Per cluster.
V0462 Per    Min II 14.0.
V0465 Per    P2 = 0.030d is superimposed.
V0466 Per    Superposition of P1 = 5300d +- 250d, P2 = 475d +- 35d
V0466 Per    (Delta(m) = 1.1m), P3 = 0.26d (Delta(m) = 0.5).
V0468 Per    P1 = 925s, P2 = 1022s. mu = 0".29, p = 170deg.
V0469 Per    Changes of line profiles with periods 0.150d, 0.188d,
V0469 Per    0.304d, 0.476d, 0.608d, 1.88d [09814].
V0469 Per    In 1978/1979 non-radial pulsations were observed:
V0469 Per    P1 = 1.74d. P2 = 2.04d [04173, 04180].
V0470 Per    VB A (B 18.8m B, 1" - 2").
V0471 Per    The central star of the planetary nebula M1-2 = VV8.
V0471 Per    According to [09815, 09816], const.
V0547 Per    High proper motion (LTT 10610) not confirmed by HIPPARCOS data.
V0580 Per    The variability may be due to the fainter (B) component.
V0582 Per    A single deep minimum at the bottom of the small-amplitude
V0582 Per    (5.63 - 5.64) wave.
V0592 Per    VB (0".2, 197 deg, 1989.7).
V0680 Per    MinII 14.07.
V0732 Per    A twice shorter period is not excluded.
V0751 Per    Min II = 11.90 :. MinII - MinI = 0.450P.
V0752 Per    Beperiodic, P2 = 0.0265d.
V0753 Per    Min II = 13.71.
V0754 Per    Min II = 12.30. MinII - MinI = 0.412P.
V0756 Per    Min II = 12.90.
V0757 Per    Multiperiodic. The range is in the Geneva B passband. VB A (B 12.2mV, 7", 185deg, 2007).
V0758 Per    Min II = 10.70.
V0789 Per    Min II = 13.4.
V0871 Per    Min II = 11.38.
V0873 Per    Min II = 11.5.
V0874 Per    VB AB (4", 215deg, 1998).
V0876 Per    Min II = 14.1.
V0877 Per    Min II = 14.0.
V0880 Per    Min II = 13.7. Type EA with D = 0.11P is not excluded.
V0881 Per    Min II = 11.01. O'Connell effect.
V0882 Per    Min II = 12.10.
V0884 Per    Min II = 11.21.
V0885 Per    Min II = 13.45.
V0886 Per    Min II = 14.1.
V0887 Per    Min II = 10.30.
V0888 Per    A twice longer period is possible.
V0889 Per    Multiperiodic. SB, Porb = 31.9456d.
V0890 Per    Min II = 12.05.
V0894 Per    Min II = 10.95. Type EB is not completely excluded.
V0899 Per    Min II = 13.17.
V0901 Per    Min II = 10.70.
V0912 Per    Min II = 12.5.
V0919 Per    VB B (A = V711 Per, 15.4mI; B 15.8mI, 8", 321deg, 1999).
V0920 Per    VB A (B = V716 Per, 14.1m, 9", 293deg, 1999).
V0929 Per    Outside the cluster tidal radius.
V0930 Per    Outside the cluster tidal radius.
V0931 Per    Outside the cluster tidal radius.
V0932 Per    Outside the cluster tidal radius.
V0934 Per    Min II = 15.85. O'Connell effect.
V0935 Per    Outside the cluster tidal radius.
V0936 Per    Min II = 15.2.
V0939 Per    Outside the cluster tidal radius.
V0943 Per    Outside the cluster tidal radius.
V0944 Per    Min II = 16.78. Outside the cluster tidal radius.
V0945 Per    Min II = 16.20. Outside the cluster tidal radius.
V0947 Per    Min II = 13.95.
V0951 Per    Min II = 13.14.
V0958 Per    A twice longer period is possible.
V0959 Per    Min II = 10.7 :.
V0960 Per    Min II = 11.83.
V0963 Per    Min II = 13.7.
V0964 Per    Min II = 12.90.
bet   Per    Multiple system (Eclipsing pair = Algol AB; Algol C 4.7m,
bet   Per    Am, a = 0".10, Porb = 1.862a); Algol AB = ADS 2362 A
bet   Per    (B 12.7m, 57".5, 156deg, 1920). P var. P = 2.8673442d
bet   Per    (1784 - 1835); P = 2.8673012d (1835 - 1854);
bet   Per    P = 2.8672775d
bet   Per    (1854 - 1901); P = 2.8672967d (1901 - 1913);
bet   Per    P = 2.8672506d
bet   Per    (1913 - 1915) [06156]; Min I = 2424477.806 + 2.86730236d*E
bet   Per    (JD2420500 - 25000); Min = 2425917.203 + 2.86732697d*E
bet   Per    (JD2425000 - 277000); Min I = 2433194.454 + 2.86731667d*E
bet   Per    (JD2427700 - 33600); Min I = 2433928.4944 + 2.86732442d*E
bet   Per    (JD2433600 - 37000); Min I = 2437598.6766 + 2.86733732d*E
bet   Per    (JD2437000 - 42200); since JD2442200 - see Table.
bet   Per    Porb (Algol C) = 1.862a may be traced in the deviations;
bet   Per    a period of 32a may also be real. Depth of Min I var.
bet   Per    Variable polarization, changes in hydrogen line profiles,
bet   Per    sometimes emissions in the spectrum. Radio source with
bet   Per    frequent burst of different amplitude, faint X-ray source.
del   Per    Variable emission lambda 1650 A [06905]. Vr var,
del   Per    A = 16 km/s.
ksi   Per    In the far IR range (lambda = 10 mkm) Delta(m) > 1m. In
ksi   Per    the far IR range (lambda = 10 mkm ) Delta(m) > 1m; the
ksi   Per    variability is related to mass loss.
omi   Per    VB A (B 8.4m, 0.96'', 29.7deg,1972). Possible
omi   Per    superposition of BCEP type oscilations.
rho   Per    A slower variation of the mean light is possible.
rho   Per    mu alpha = 0.0111s, mu delta = -0.102''.
phi   Per    SB2. (Porb = 126.696d). v*sin(i) = 450km/s. A var (P ~Porb).
b     Per    SB2. Depths of minima differ by 0.03m. Third body? ,
b     Per    P = 701d. Radio source. In  the region of the open cluster
b     Per    NGC 1545.
R     Phe    P var. Max = 2405121 + 271.0d*E(JD2405000 - 11500);
R     Phe    Max = 2414570 + 266.26d*E(JD2414500 - 25500);
R     Phe    since JD2425500 - see Table.
T     Phe    P var. Max = 2411252 + 281.00d*E(JD2410000 - 30000);
T     Phe    since JD2430000 - see Table.
W     Phe    P var. Max = 2414960 + 328.65d*E(JD2414500 - 19500);
W     Phe    Max = 2424530 + 332.87d*E(JD2424500 - 30200);
W     Phe    since JD2436000 - see Table.
RS    Phe    P var?
RT    Phe    P = 208d?
RV    Phe    P var?; (k-b)2 = 0.06; Delta(S) = 8:
SX    Phe    mu = 0.894", ro = 163.1deg. P var. Max = 2433923.9618 +
SX    Phe    0.054964519d*E1 - 0.00337d*sin(2pi*(0.28503379*E1 + 0.074))
SX    Phe    (JD2433900 - 36900); since JD2436900 - see Table.
SX    Phe    There is a periodic term in the elements given in the
SX    Phe    Table: -0.00325*sin(2pi*(0.28503575*E2 - 0.107)). According
SX    Phe    to [09614] for epoch 1950.0 P0 = 0.054964509,
SX    Phe    P1 = 0.042772831, Pb = 0.1928355; dP0/dt = -87*10**(-13),
SX    Phe    dP1/dt = -174*10**(-13), dPb/dt = 2.46*10**(-10).
SX    Phe    P1/P0 = 0.778; 0.8m <= A <= 0.3m;
SX    Phe    0.2p <= M-m <= 0.4p. [Fe/H] = -0.6.
WW    Phe    Min II 12.7.
YZ    Phe    Min II 13.0.
AD    Phe    Min II 10.80. P var. Min I = 2436847.375 + 0.3799277*E
AD    Phe    (JD2428650 - 36850); since JD2436850 - see Table.
AE    Phe    Min II 8.19; 0.033p <= dI <= 0.05p; dII = 0.00.  The
AE    Phe    shape of the light curve varies with periods 55.9d and
AE    Phe    95.3d [09615]. P var. Min I = 2440857.8140 + 0.36237459*E
AE    Phe    (JD2438250 - 40870) [07388]; Min I = 2441969.57074 +
AE    Phe    0.36237186d*E (JD2440870 - 42000) [09616]; Min I =
AE    Phe    2442654.8201 + 0.3623741d*E (JD2441950 - 42660) [09533];
AE    Phe    since JD2443700 - see Table.
AG    Phe    Min II 8.95. P var. Min I = 2440415.231 + 0.7553429d*E
AG    Phe    (JD243800 - 40850); since JD2443750 - see Table.
AI    Phe    Min II 8.89; dI = 0.0035; Min II - Min I = 0.46p.
AU    Phe    Min II 13.0. According to [09517] the P value given in
AU    Phe    the Table is wrong.
AX    Phe    mu = 0.234", p = 70deg. Multiperiodical: P i = 606.8s,
AX    Phe    682.7s, 744.7s, 840.2s (Ai ~0.01m).
CG    Phe    Type RRC: is also possible.
CZ    Phe    The first-overtone period is tabulated. P0 = 0.56680d, Delta(m)1/Delta(m)0 = 1.9.
gam   Phe    SB1 (P orb = 193.85d).
zet   Phe    VB A (B 7.0m, A7:, 0.46", 51.4deg, 1965.9; C 8.0m,
zet   Phe    F7V, 6.4"). Total light range of A and B components is
zet   Phe    given in the Table. Min II 4.22, MinII - MinI = 0.507p;
zet   Phe    dII = 0.02p.
iot   Phe    VB A (B 12.7m, 7.7", 270deg).
ksi   Phe    VB A (B 12.1m, 13.2", 253deg). Epoch of MinI(v) is given
ksi   Phe    in the Table. A(v) = 0.13m.
rho   Phe    Frequency analysis results see also in [09619, 09620, 9621].
psi   Phe    SB.
R     Pic    P var. Max = 2413413  +  165.8d*E (JD2413000 - 23600);
R     Pic    since JD2423600 - see Table. Light curve (1923 - 1953)
R     Pic    [01054].
S     Pic    P var. Max = 2413595  +  424.7d*E (JD2405500 - 23000);
S     Pic    since JD2423000 - see Table. OH emission.
U     Pic    P var. Max = 2428103.565  +  0.44036450*E (JD2414000 -
U     Pic    29000) [00353]; since JD2438400 - see Table. (k - b)2 =
U     Pic    0.17; Delta(S) = 3.
X     Pic    Min II 10.8
RR    Pic    Since 1965 periodic light variations were detected
RR    Pic    with A(B) = 0.33m and elements Max = 2438815.380 +
RR    Pic    0.14502545d*E. These variations are superimposed by
RR    Pic    others with A(B) = 0.036m and period ~15.6 min or
RR    Pic    15.4 min [09612]. There are also rapid oscillations
RR    Pic    with periods in the range 20 - 40s [09613].
RT    Pic    Not seen only on one plate; defect?
RV    Pic    Min II 9.79.
SU    Pic    Min II 10.4.
VW    Pic    Variability may be due to component B.
VZ    Pic    Kapteyn's star.
AL    Pic    Blazhko effect, P = 34.0d.
AM    Pic    VB A (A 9.6m; B = HD 273920, 10.3m, Sp K7, 27", 123deg, 2000). The tabulated range is for the combined brightness.
AO    Pic    VB (A 9.7m; B 11.1m, 2.1", 39deg, 1929).
AS    Pic    Min II = 11.10. dP/dt = +0.38 x 10^(-5)d/yr.
AU    Pic    Min II = 14.3.
del   Pic    Min II 4.83.
R     Psc    P var. Max = 2418070 + 344.14d*E (JD2397070 - 27700);
R     Psc    Max = 2432866 + 347.1d*E(JD2427300 - 33000) - see Table.
S     Psc    P var. Max = 2406665 + 405.6d*E (JD2398944 - 2407100);
S     Psc    Max = 2415930 + 402.6d*E (JD2407100 - 16500); Max =
S     Psc    2421295 + 413.7d*E (JD2416500 - 21500) - see Table.
U     Psc    P var. Max = 2417230 + 172.71d*E (JD2407720 - 18000);
U     Psc    Max = 2423840 + 174.3d*E (JD2418000 - 24000) [00001];
U     Psc    Max = 2424527 + 170.3d*E (JD2423000 - 26100) [00960];
U     Psc    Max = 2432514 + 174.05d*E (JD2425000 - 33000) [00001];
U     Psc    since JD2433000 - see Table.
V     Psc    mu alpha = 0.0112s, mu delta = -0.215".
W     Psc    P var. Max = 2412690 + 189.08d*E (JD2412692 - 27100)
W     Psc    [01193];
W     Psc    since JD2435000 - see Table.
X     Psc    P var. Max = 2433474 + 357.3*E (JD24295000 - 38000); since
X     Psc    JD2438000 - see Table.
Y     Psc    P var. Min = 2410002.844 + 3.76582d*E (JD2410000 - 19700)
Y     Psc    [09707]; Min = 2425495.522 + 3.765903d*E
Y     Psc    (JD2423200 - 6300) [01072]; Min = 2430613.384 +
Y     Psc    3.7658895d*E
Y     Psc    (JD2427300 - 30620); Min = 2432865.357 + 3.7658405d*E
Y     Psc    (JD2430620 - 32900); Min = 2435693.452 + 3.7657765d*E
Y     Psc    (JD2432860 - 36600) [00001]; Min = 2441225.473 +
Y     Psc    3.765859d*E
Y     Psc    (JD2439000 - 42500) [06956]; Min = 2443142.29056 +
Y     Psc    3.7658491d*E (JD2442500 - 44000) [08593]; since JD2444000 -
Y     Psc    see Table.
RS    Psc    In the region of the galaxy NGC 251.
RT    Psc    Mean brightness varies with P2 = 533d. According to [08643]
RT    Psc    30d <= P1 <= 70d.
RU    Psc    [Fe/H] = -1.65. P var. [00752, 09714] Max = 2415407.609 +
RU    Psc    0.3903008d*E (JD2414400 - 15700); Max = 2416022.660 +
RU    Psc    0.3902139d*E (JD2415700 - 16600); Max = 2417244.537 +
RU    Psc    0.3902878d*E (JD2416600 - 19200); Max = 2419936.853 +
RU    Psc    0.3903520d*E (JD2419200 - 22000); Max = 2425894.778 +
RU    Psc    0.3903016d*E (JD2422000 - 26200); Max = 2426214.829 +
RU    Psc    0.3903546d*E (JD2426200 - 27300); Max = 2427397.519: +
RU    Psc    0.3902216d*E (JD2427300 - 28000); Max = 2428165.524 +
RU    Psc    0.3903535d*E (JD2428000 - 29300); Max = 2429488.868: +
RU    Psc    0.3904577d*E (JD2429300 - 600) [00752]. Max = 2430053.353 +
RU    Psc    0.390202d*E (JD2430000 - 650); Max = 2430935.366 +
RU    Psc    0.390354d*E (JD2430600 - 940); Max = 2431331.307 +
RU    Psc    0.390457d*E (JD2430940 - 31350); Max = 2432119.417 +
RU    Psc    0.390346d*E (JD2431350 - 32120); Max = 2433162.250 +
RU    Psc    0.390283d*E (JD2432100 - 33200); Max = 2433905.311 +
RU    Psc    0.390261d*E (JD2433200 - 33910); Max = 2433905.311 +
RU    Psc    0.390321d*E (JD2433900 - 35430); Max = 2435429.502 +
RU    Psc    0.390412d*E (JD2435420 - 35800); Max = 2435781.265 +
RU    Psc    0.39027d*E (JD2435780 - 36130); Max = 2436501.361 +
RU    Psc    0.39032d*E (JD2436130 - 36510); Max = 2436534.190 +
RU    Psc    0.39043d*E (JD2436500 - 36850); Max = 2436845.351 +
RU    Psc    0.39025d*E (JD2436840 - 37200); Max = 2437181.358 +
RU    Psc    0.39031d*E (JD2437180 - 37610); Max = 2437994.329 +
RU    Psc    0.39026d*E (JD2437610 - 38000); [00001].
RU    Psc    Max = 2438303.950 + 0.39040d*E (JD2438000 - 38400) [03879].
RU    Psc    Max = 2438375.409 + 0.39027d*E (JD2438370 - 38650) [00001].
RU    Psc    Max = 2439435.2421 + 0.390385d*E (JD2438650 - 39500)
RU    Psc    [09713]. Max = 2439435.242 + 0.390313d*E (JD2439430 - 39800);
RU    Psc    Max = 2439771.3049 + 0.39046d*E (JD2439770 - 40140) [00001].
RU    Psc    Since JD2440140 - see Table. According to [03569] A var
RU    Psc    with P = 28.8d.
RV    Psc    Min II 12.0.
RY    Psc    (k-b)2 = 0.03, Delta(S) = 7. P var. Max = 2419677.268 +
RY    Psc    0.52971027d*E (JD2414000 - 22000); Max = 2425148.192 +
RY    Psc    0.52972643d*E (JD2422000 - 25500) [01337]; Max =
RY    Psc    2425508.390 + 0.5297291d*E (JD2425500 - 40000);
RY    Psc    Max = 2441538.476 + 0.52972911d*E (JD2441000 - 41650)
RY    Psc    [07984]; since JD2442660 - see Table.
RZ    Psc    Algol-like.
SS    Psc    (k-b)2 = 0.19; Delta(S) = 2. Blazhko effect:
SS    Psc    -0.04d <= O-C <= +0.04d; Min(O-C) = 2437520 + 136d*E
SS    Psc    [09731].
SU    Psc    Min II 11.3.
SW    Psc    P var. Max = 2425177.298 + 0.5212844d*E (JD2419670 -
SW    Psc    25200) [04191]; Max = 2425177.256 + 0.5212642d*E
SW    Psc    (JD2425170 - 38000) [03506]. Since JD2438600 - see Table.
SW    Psc    There is a periodic term in the elements given in the
SW    Psc    Table: + 0.0132d*sin(5.440deg*(E + 2)). Blazhko effect
SW    Psc    (Pi = 34.5d).
SX    Psc    P var. Min = 2427811.357 + 0.825882d*E (JD2425580 - 36000)
SX    Psc    [01218]; Min = 2437202.453 + 0.825877d*E
SX    Psc    (JD2436000 - 39900)
SX    Psc    [00001]; since JD2439800 - see Table.
SZ    Psc    Min II 7.38. P var.
SZ    Psc    There is a square term in the elements given in the Table:
SZ    Psc    -0.113d*10**(-6)*E**2.
TY    Psc    Porb = 0.080d [09735].
TY    Psc    The cycle of supermaxima is 370d [09675].
UU    Psc    VB A (B 7.60m, F4V, 11.5", 148deg, 1966.9). Min II 6.04;
UU    Psc    Min II - Min I = 0.55P.
UU    Psc    Elliptical orbit and rotation of the line of apsides are
UU    Psc    possible.
UV    Psc    Min II 9.54. P var. Min I = 2424134.574 + 0.8610475d*E
UV    Psc    (JD2414600 - 24150) [00001]; Min I = 2428038.555 +
UV    Psc    0.861046d*E (JD2424150 - 36700) [02924];
UV    Psc    since JD2436700 - see Table. The shape of the light
UV    Psc    curve varies.
UW    Psc    Min II 11.0:.
UZ    Psc    SB1 (Porb > 1 yr [05751]).
VZ    Psc    Mu = 0.43", P =  65deg. Min II 10.43.
WW    Psc    VB A (B 13.1m, 31").
WX    Psc    OH, H2O, SiO maser.
ZZ    Psc    P1 = 612s, P2 = 816s [07476].
ZZ    Psc    Nonradial modes [08467].
AG    Psc    P (Vr) = 0.055d.
AH    Psc    The star was seen in 1854 - 60; since 1862 it was not
AH    Psc    observed.
AO    Psc    Epoch of Max brightness is given. Light variations with
AO    Psc    Porb = 0.1496263d are superimposed by variations with
AO    Psc    P = 858.6861s and twice smaller amplitude (Max =
AO    Psc    2444815.00276 + 0.009938496d*E; M-m = 0.54P), and
AO    Psc    also by still smaller oscillations with P = 805.2059s
AO    Psc    (Max = 2444815.00294 + 0.009319513d*E). The last period
AO    Psc    is the X-ray impulse period which is equal to
AO    Psc    the period of rotation of the compact object (probably
AO    Psc    a white dwarf).
EM    Psc    The depth of MinII is 0.35.
EQ    Psc    Multi-mode pulsations at a time scale of hours.
ET    Psc    VB (A 9.1m; B 11.8m, 2".9, 198deg, 1830).
EU    Psc    VB (A 9.1m; B 9.8m, 0.1", 111deg, 1991).
EW    Psc    Min II = 10.37.
EX    Psc    Min II = 14.27.
EY    Psc    Min II = 9.35 :.
EZ    Psc    VB A (B 13.6m, 25", 59deg, 2000; C 12.1m, 33", 131deg, 1969).
FM    Psc    Multiperiodic.
FR    Psc    Blazhko effect, P=51d:.
FT    Psc    VB AB (A 12.5mHp; B 13.6mHp, 2", 316deg, 1991).
FU    Psc    Min II = 11.98 :.
FY    Psc    Min II = 13.3.
GG    Psc    Min II = 13.85.
GK    Psc    Min II = 13.9.
GO    Psc    Min II = 13.35.
GR    Psc    Min II = 11.75.
GS    Psc    VB A (B 15.8mV, 10", 62deg, 1997).
GT    Psc    Min II = 12.47.
GW    Psc    Min II = 12.0.
GX    Psc    Min II = 13.65.
GY    Psc    Min II = 12.6.
HL    Psc    Min II = 10.97. Strong O'Connell effect in [021] but not in [057].
HN    Psc    Min II = 10.93.
HO    Psc    Min II = 11.6.
IN    Psc    VB A (B 8", 48deg, 1999). Combined magnitudes are tabulated.
R     PsA    P var. Max = 2417385 + 293.00d*E (JD2405000 - 26000);
R     PsA    Max = 2432896 + 291.50d*E (JD2426000 - 38000);
R     PsA    since JD2438000 - see Table.
S     PsA    P var. Max = 2417853 + 271.0d*E (JD2411000 - 18000);
S     PsA    Max = 2426880 + 273.6d (JD2418000 - 27000); Max =
S     PsA    2434714 + 270.3d (JD2427000 - 35000); since
S     PsA    JD2434000 - see Table.
X     PsA    Min II 14.2.
RW    PsA    Min II 11.63.
TX    PsA    VB B (A 13.0m pg; B 37", 131deg); mu = 0.22", p = 117deg.
XZ    PsA    MinII 8.04.
AE    PsA    Blazhko effect, P = 5.78d.
AG    PsA    The first-overtone period is tabulated. P0 = 0.49785d. A1/A0 = 1.6.
pi.   PsA    SB (Porb = 178.3177d [05769]).
R     Pup    In the region of the open cluster NGC 2439.
U     Pup    P var. Max = 2415090 + 314.26d*E (JD2408000 - 22800);
U     Pup    since JD2422800 - see Table.
V     Pup    VB A (B 10.0m, 7", 0, 70deg; C 11.0m, 19.0", 48deg).
V     Pup    Min II 4.82. P var. IO - CI < 0.02d.
W     Pup    P var. Max = 2420990 + 120.68d*E (JD2412500 - 23600);
W     Pup    Max = 2424725 + 119.9d*E (JD2423600 - 26300);
W     Pup    Max = 2432200 + 120.68d*E (JD2426300 - 40800);
W     Pup    since JD2440800 - see Table.
X     Pup    P var. Max = 2414889.8 + 25.939d*E (JD2408800 - 16000);
X     Pup    Max = 2435188.76 + 25.9610d*E (JD2419000 - 35190)
X     Pup    [02392]; Max = 2436279.50 + 25.97d*E
X     Pup    (2435190 - 38000) [00001]; since JD2438000 - see Table.
Z     Pup    OH, H2O, SiO emission.
Z     Pup    P var. Max = 2424256 + 513.90d*E (JD2413900 - 24500);
Z     Pup    since JD2424500 - see Table.
RS    Pup    Surrounded by the reflecting nebulosity with a radius of
RS    Pup    1.4' [09634]. P var. Max = 2419186.3 + 41.337d*E
RS    Pup    (JD2414000 - 24000) [02049]; Max = 2427083.613 + 41.414d*E
RS    Pup    (JD2425800 - 28300) [02440]; Max = 2434823.23 + 41.38535d*E
RS    Pup    (JD2433750 - 34900) [09636]; since JD2435700 - see Table.
RW    Pup    P var. Max = 2430175 + 332.5d*E (JD2424500 - 30200)
RW    Pup    [00001]; since JD2435800 - see Table.
RX    Pup    Light curve (1890 - 1925) [01265].
RX    Pup    Mira type component light variations are observed in the
RX    Pup    infrared region of spectrum: Max = 2444530 + 580d*E,
RX    Pup    3.99m - 6.00m J, M - m = 0.50P [09518].
ST    Pup    [A/H] = -0.9.
ST    Pup    The light curve shape and the period vary strongly:
ST    Pup    0.10P < M - m < 0.30P; 17.4d < P < 19.19d.
ST    Pup    P = 19.188d (JD2415000 - 17000); 18.949d
ST    Pup    (JD2417000 - 18000), 18.8065d (JD2418000 - 19000),
ST    Pup    18.721d (JD2419000 - 20000), 18.714d (JD2420000 - 21000),
ST    Pup    18.717d (JD2421000 - 22000), 18.6175d (JD2422000 - 23000),
ST    Pup    18.678d (JD2423000 - 24000), 18.735d (JD2424000 - 25000),
ST    Pup    18.796d (JD2425000 - 26000), 18.817d (JD2426000 - 27000)
ST    Pup    [01266]. Max = 2427779.6 + 18.846d*E (JD2427000 - 28000)
ST    Pup    [01266]; Max = 2428893.9 + 18.885d*E (JD2428000 - 29000)
ST    Pup    [00016]; Max = 2429697.51 + 19.188d*E (JD2429000 - 30000)
ST    Pup    [01266]. P = 19.142d (JD2430000 - 31000),
ST    Pup    19.145d (JD2431000 - 32000) [01266].
ST    Pup    Max = 2435395.430 + 18.559d*E (JD2435160 - 500)
ST    Pup    [06006]; Max = 2435617.45 + 18.8864d*E (JD2435500 - 5620)
ST    Pup    [02309]; Max = 243957.3 + 17.4d*E (JD2438700 - 39600)
ST    Pup    [06611]; since JD2444000 - see Table.
SV    Pup    P var. Max = 2419010 + 166.6d*E (JD2413660 - 18000);
SV    Pup    Max = 2423090 + 169.8d*E (JD2418000 - 23100);
SV    Pup    Max = 2426782 + 167.8d*E (JD2423100 - 27500);
SV    Pup    since JD2427500 - see Table.
SW    Pup    Min II 9.1; d = 0.029P.
TT    Pup    Min II 13.6.
TY    Pup    Min II 8.87.
UZ    Pup    Min II 10.0.
VV    Pup    mu = 0.100", P = 165.0deg.
VV    Pup    The epoch of light maximum is given. The mean
VV    Pup    brightness varies by 2 - 3m. Intervals of active light
VV    Pup    variation with amplitude up to 2m during maximal mean
VV    Pup    brightness are observed. During low activity intervals
VV    Pup    when amplitude is about 0.3m mean brightness is minimal;
VV    Pup    during this time the ellipsoidal light variations of the
VV    Pup    system are observed in the range 15.1m - 15.3m J with the
VV    Pup    elements Min = 2427889.6509 + 0.0697468256d*E [09644].
VV    Pup    The white dwarf rotation period is equal to the orbital
VV    Pup    period. There are flickerings. Spectrum description
VV    Pup    [09472, 09645].
VW    Pup    P var. Max = 2425184.67 + 4.28405d*E (JD2422660 - 25600)
VW    Pup    [00973]; Max = 2435554.86 + 4.28519d*E (JD2425600 - 35600)
VW    Pup    [02309]; since JD2435500 - see Table.
VX    Pup    P1 = 2.1389d (A1 = 0.29m); A0 = 0.31m; P1/P0 = 0.71042.
VY    Pup    The depth of Min II 0.04m.
VZ    Pup    [A/H] = -0.3. P var. Max = 2434864.90 + 23.1640d*E
VZ    Pup    (JD2426700 - 35300) [02309]; since JD2435300 - see Table.
WW    Pup    P var. Max = 2424497.73 + 5.5159d*E (JD2423520 -
WW    Pup    26000) [00973]; since JD2426000 - see Table.
WX    Pup    P var. Max = 2435042.184 + 8.93825d*E (JD2422000 -
WX    Pup    35100) [02431]; since JD2435000 - see Table.
WZ    Pup    P var. Max = 2427861.33 + 5.02657d*E (JD2421100 -
WZ    Pup    29400) [02392]; since JD2429400 - see Table.
XX    Pup    P var. Max = 2426338.503 + 0.51719805d*E
XX    Pup    (JD2426300 - 39500) [03572]; since JD2441700 - see Table.
XX    Pup    (k - b)2 = 0.07. The spectral type according to CA II is
XX    Pup    given.
XY    Pup    Min II 9.4; d = 0.042P.
XZ    Pup    Min II 7.90. P var. Min I = 2440629.7969 + 2.192383d*E
XZ    Pup    (JD2425850 - 41700) [00099]; since JD2441700 - see Table.
YY    Pup    The depth of Min II 0.05m.
AE    Pup    In the region of the open cluster Cr 173.
AF    Pup    Min II 13.5.
AG    Pup    Min II 10.9.
AH    Pup    The depth of Min II 0.05m.
AN    Pup    Min II 10.7.
AQ    Pup    VB A (B 11.13m, < 15"; C 12.83m, < 15"). [A/H] = -0.1.
AQ    Pup    The range of the variation of combined light is given.
AQ    Pup    P var. Max = 2429734.59 + 29.931d*E (JD2427500 - 33000)
AQ    Pup    [03474]; Max = 2433296.2 + 30.018d*E (JD2433000 - 35850)
AQ    Pup    [02474]; Max = 2436625.9 + 29.8568d*E
AQ    Pup    (JD2435850 - 36700) [03601]; Max = 2441760.63 + 30.032d*E
AQ    Pup    (JD2436600 - 42700) [09671]; since JD2443400 - see Table.
AR    Pup    The mean brightness varies with P = 1200d.
AS    Pup    In the region of the open cluster NGC 2546. P var.
AS    Pup    Max = 2416110 + 331.4d*E (JD2415460 - 26000); since
AS    Pup    JD2426000 - see Table.
AT    Pup    In the region of the open cluster NGC 2546.
AT    Pup    P var. Max = 2426758.205 + 6.6648d*E (JD2426700 - 35600)
AT    Pup    [02202]; since JD2435600 - see Table.
AU    Pup    Min II 9.28. P var. Min I = 2428111.304 + 1.126418d*E
AU    Pup    (JD2414700 - 28200) [00007]; since JD2439000 - see Table.
AV    Pup    Min II 11.0.
AW    Pup    VB A (B 11.7m, 3.7", 258deg). Period probably must be
AW    Pup    doubled.
AY    Pup    Min II 12.5.
AZ    Pup    Min II 10.1.
BB    Pup    (k - b)2 = 0.24; Delta(S) = 3.
BH    Pup    In the region of the open cluster Cr 173.
BI    Pup    In the region of the open cluster Cr 173.
BK    Pup    In the region of the open cluster Cr 173.
BL    Pup    Min II 14.2.
BN    Pup    In the region of the open cluster NGC 2533.
BP    Pup    Min II 12.3.
BQ    Pup    The shape of the light curve possibly varies.
BR    Pup    Min II 12.9.
BT    Pup    Min II 14.5. In the region of the open cluster NGC 2482.
BU    Pup    Min II 13.9. In the region of the open cluster NGC 2447.
BW    Pup    The depth of Min II 0.15m.
BX    Pup    In the region of the open cluster NGC 2482.
CE    Pup    P var? [07934].
CH    Pup    P var. Max = 2428465 + 491.0d*E (JD2428400 - 37300);
CH    Pup    since JD2437300 - see Table.
CO    Pup    P var? The epoch of light minimum is given.
CP    Pup    In 1981 the radius of the shell expanding with
CP    Pup    Vexp = 710 km/s was equal to 7" [09689, 09559].
CX    Pup    d = 0.05P.
CY    Pup    d = 0.01P:; Min II 13.0.
CZ    Pup    Min II 13.1.
DD    Pup    Min II 14.6; Min II - Min I = 0.572P.
DE    Pup    Min II 12.9.
DF    Pup    Min II 12.8.
DK    Pup    Min II 13.0.
DM    Pup    Min II 13.7; Min II - Min I = 0.62P.
DN    Pup    Min II 13.5.
DO    Pup    Min II 13.3.
DR    Pup    Min II 13.3:.
DS    Pup    Min II 13.4.
DT    Pup    Min II 14.3.
EK    Pup    VB A (B 15", 270deg). P var? Max = 2427747.89 + 2.62587d*E
EK    Pup    (JD2425500 - 29500) [01343]; since JD2434500 - see Table.
EL    Pup    P > 1.3d? In the region of the open cluster NGC 2437.
EN    Pup    Min II 11.4.
EQ    Pup    Min II 10.9.
ES    Pup    According to [00412], Max = 2430377 + 187d*E.
ES    Pup    The elements given in the Table are valid in the interval
ES    Pup    JD2425600 - 29700.
EU    Pup    Min II 14.8.
FK    Pup    A var (P2 = 3000d). Strong SiC2 bands in the spectrum.
FM    Pup    Min II 14.2.
GG    Pup    S5/5.
GH    Pup    VB A (B 10", 195deg; C 16", 280deg; D 14", 315deg). P var.
GH    Pup    Max = 2425450 + 800d*E (JD2425300 - 28000); since
GH    Pup    JD2428700 - see Table. Very red.
GI    Pup    In the region of the open cluster NGC 2437.
GK    Pup    IN the region of the open cluster NGC 2437.
GN    Pup    VB A (B 16.5m, 10", 80deg).
GP    Pup    Min II 13.5.
GU    Pup    Min II 12.2.
GX    Pup    Min II 13.9. In the region of the open cluster Cr 173.
GY    Pup    Min II 12.3.
GZ    Pup    Min II 12.1.
HH    Pup    (k - b)2 = 0.14, Delta(S) = 1.
HI    Pup    Min II 11.0. In the region of the open cluster Cr 173.
HK    Pup    P var. Max = 2425925.732 + 0.7342532d*E
HK    Pup    (JD2425300 - 36600) [04127]; since JD2436600 - see Table.
HM    Pup    There is a shallow Min II.
HP    Pup    P var?
HW    Pup    P var? Max = 2429756.28 + 13.4532d*E (JD2427100 - 33000)
HW    Pup    [03551]; since JD2433000 - see Table.
KQ    Pup    In the open cluster NGC2422. SB2 (Porb = 9752d [03985]).
KT    Pup    Min II 13.4.
KW    Pup    Min II 11.8.
KX    Pup    Min II 13.04; 0.435P (1930) < Min II - Min I < 0.56P (1973)
KX    Pup    [03474, 08094]; e = 0.15. Apsidal motion.
KY    Pup    Min II 11.1.
LN    Pup    Min II 12.9; Min II - Min I = 0.533P.
LO    Pup    Min II 13.9.
LP    Pup    d = 0.03P:.
LT    Pup    Min II 12.6.
MN    Pup    Min II 13.2.
MQ    Pup    Min II 9.39.
MT    Pup    RCB?
MW    Pup    Min II 9.2.
NO    Pup    VB A [BC 7.19m V, 8.1". 124deg (delta(M) = 0.0m, 0.20",
NO    Pup    275deg,
NO    Pup    1976)]. Min II 6.66; Min II - Min I = 0.582P; e = 0.123.
NQ    Pup    S 4.5/2-.
NW    Pup    Porb = 1d.
NX    Pup    Connected with a cometary nebula.
OR    Pup    In the region of the open cluster NGC 2467.
OS    Pup    VB A (B 6.10m, 67.4").
OS    Pup    In the region of the open cluster C 0812-362.
OU    Pup    In the region of the open cluster IC 2391.
OX    Pup    In the region of the open cluster NGC 2451.
PS    Pup    The depth of Min II 0.028m.
PT    Pup    P2 = 0.168377d. A (lambda 1550) = 0.043m;
PT    Pup    0.015m < A(B) < 0.035m.
PU    Pup    VB (5.2m, 5.6m; 0.11", 43.6deg, 1927). Min II 4.74.
PV    Pup    VB B (A 6.1m; B 16.9", 340deg; C 10.5m, 100.4", 228deg).
PV    Pup    Min II 7.31; DII 0.10P; Min II - Min I = 0.47P.
PV    Pup    The light curve shape in Max and Min II varies.
PV    Pup    The deviations DB from the mean curve vary from -0.06m
PV    Pup    to +0.03m with the elements: Max (IDelta(B)I) =
PV    Pup    2440000.027458 + 1.92207d*E or Max (IDelta(B)I) =
PV    Pup    2440000.219470 + 0.48003d*E.
PW    Pup    Min II 9.54; d = 0.095P. In the region of the open
PW    Pup    cluster NGC 2439.
QS    Pup    0.008m <= A(u) <= 0.015m.
QT    Pup    Probably a member of the open cluster NGC 2477.
QU    Pup    P2 = 0.1680d or 0.2019d; 0.010m <= A(u) <= 0.040m.
QV    Pup    May be a member of the open cluster NGC 2489.
V0360 Pup    Type ACV: is also possible.
V0364 Pup    The preceding component of the northern star in the system of two
V0364 Pup    CoD-CPD objects, COD-36 3425 and CoD-36 3426 (CPD-36 1171 and CPD-36
V0364 Pup    1172).  The cross-identifications of these CoD and CPD objects differ
V0364 Pup    from one source to another; our adopted identification is based on the
V0364 Pup    paper editions of the catalogs.
V0376 Pup    Type ACV: is also possible.
V0378 Pup    Type BE is also possible.
V0393 Pup    SB, Porb = 2.5248d.
V0419 Pup    Not a nearby star (despite having a Gl number).
V0575 Pup    VB, rho=2". Component A: SB.
V0579 Pup    MinII 13.52.
V0581 Pup    MinII 12.43.
V0582 Pup    MinII 7.94:.
V0587 Pup    MinII 9.25. Erroneously marked in the chart in [321].
V0588 Pup    The chart in [107] is assumed to be wrong.
V0589 Pup    MinII 8.97.
V0596 Pup    VB A (B 8.58m, 0.3").
V0596 Pup    Range of the variation of combined light is given.
V0596 Pup    Min II 7.03; DII = 0.08P; Min II - Min I =
V0596 Pup    0.48P. Min II = 2444622.86709 + 4.5961766d*E.
V0596 Pup    Apsidal motion (P = 3200 yr).
V0605 Pup    A twice shorter period is not excluded.
V0611 Pup    MinII - MinI = 0.40P. VB (A 8.6m; B 9.1m, 0.3", 130deg, 1990).
V0620 Pup    VB B (A 11.7mV; B 12.0mV, 28", 358deg, 1999; C 12.5mV, 16", 78deg, 1999).
V0624 Pup    A much longer cycle superposed.
V0626 Pup    VB (A 9.65m; B 10.0m, 9", 55deg, 1991).
V0628 Pup    VB A (B 15.8mpg, 9", 84deg, 1995).
V0634 Pup    A twice longer period is not excluded.
V0642 Pup    MinII - MinI = 0.6P.
V0651 Pup    Min II = 12.4.
V0652 Pup    Min II = 9.83. VB AB (A 10.44m; B 10.55m, 0.80", 170deg, 1991). P varies. dP/dt = -0.28 x 10^(-5) d/yr.
V0653 Pup    Min II = 10.53.
V0654 Pup    Min II = 14.8.
V0656 Pup    Min II = 18.25.
V0658 Pup    Min II = 16.76.
V0660 Pup    Min II = 16.4 :.
V0661 Pup    Min II = 20.7.
V0662 Pup    Min II = 20.5.
V0663 Pup    Min II = 17.32:.
V0664 Pup    Min II = 12.25. P varies. dP/dt = +0.24 x 10^(-5) d/yr.
V0667 Pup    VB (1.8"), the NE star of the pair varies. The tabulated period is probably orbital. Stable pulses with Pspin = 0.00593d and amplitude of 0.03m.
V0668 Pup    Min II = 13.3.
V0670 Pup    Min II = 9.00. Eclipse amplitude is about 0.06m , out-of-eclipse variations [80015] with an amplitude about 0.12m.
V0674 Pup    Min II = 10.95. P varies. dP/dt = -0.77 x 10^(-5) d/yr.
V0675 Pup    Min II = 10.9.
V0683 Pup    Multiperiodic. P2 = 1.40294d, P3 = 1.17811d.
V0687 Pup    Blazhko effect?
V0690 Pup    Min II = 8.96.
V0691 Pup    Min II = 12.53.
V0692 Pup    Min II = 14.70.
V0695 Pup    Min II = 15.85.
V0696 Pup    Min II = 14.39.
V0697 Pup    Min II = 11.06. Cluster non-member.
V0698 Pup    Min II = 12.6.
V0701 Pup    Two modes with similar amplitudes. For the second mode, Max = 2453015.749 + 0.296111d x E.
omi   Pup    Type EA: is also possible.
rho   Pup    VB A (B 13.7m, 29.6", 15deg). [Fe/H] = +0.13. P var.
rho   Pup    Max = 2435552.807 + 0.14088141d*E (JD2413900 -
rho   Pup    37500) [09756]; Max = 2439887.843 + 0.14088141d*E
rho   Pup    (JD2439800 - 43700); since JD2444000 - see Table.
L   2 Pup    VB A (B 11.5m, 62", 214deg); mu = 0.34", P=18deg. H2O,
L   2 Pup    SiO maser.
S     Pyx    P var. Max = 2411770 + 206.60d*E (JD2405500 - 23700);
S     Pyx    Max = 2423765 + 207.0d*E (JD2423700 - 29600);
S     Pyx    since JD2429600 - see Table.
T     Pyx    Previous outbursts were observed in 1890, 1902, 1920, 1944.
RR    Pyx    A close companion 14.5m.
RZ    Pyx    Min II 9.69.
SU    Pyx    d = 0.016P.
TT    Pyx    P = 3.031556d?
TV    Pyx    Depth of Min II 0.05m.
TX    Pyx    Min II 9.8.
TY    Pyx    Min II 7.48.
TZ    Pyx    Min II 11.1.
UZ    Pyx    VB A (B 7.61m, 110", 180deg).
VW    Pyx    The nucleus of the planetary nebula K1-2.
VW    Pyx    The range of the variations of combined light:
VW    Pyx    15.7 - 17.4 pg. The value of P close to
VW    Pyx    that found by bond [09767] and the epoch of Max brightness
VW    Pyx    are given in the Table.
CR    Pyx    MinII 11.37.
CU    Pyx    MinII 12.36.
CY    Pyx    SB1.
CZ    Pyx    P = 635d [130] superimposed.
DK    Pyx    MinII - MinI = 0.29P.
DN    Pyx    A twice shorter period is not excluded.
DQ    Pyx    Min II = 9.31.
R     Ret    P var. Max = 2403013 + 280.0d*E (JD2403000 - 13900);
R     Ret    Max = 2423317 + 276.68d*E (JD2413900 - 25300);
R     Ret    Max = 2430008 + 279.7d*E (JD2425200 - 30020);
R     Ret    since JD2430000 - see Table.
T     Ret    Mean brightness varies with P = 200d.
X     Ret    (k - b)2 = 0.09. P var. Max = 2427425.47 + 0.4920d*E
X     Ret    [00357]; Max = 2434334.611 + 0.492011d*E (JD2434300 - 600)
X     Ret    [00080]; since JD2434600 - see Table.
X     Ret    The shape of the light curve varies. Blazhko effect:
X     Ret    Pi >= 45d; 0.13P <= M - m <= 0.23P [00080].
VY    Ret    MinII - MinI = 0.75P.
WY    Ret    Min II = 14.0.
R     Sge    P var (70.07d <= P <= 71.24d [09769]. Period variation
R     Sge    study [00767]. The elements given in the Table are valid
R     Sge    since JD2434000. The mean brightness varies:
R     Sge    Min = 2414402 + 1112.d*E [01357].
S     Sge    SB1 (Porb = 675d [01358]). P var. Max = 2409863.32 +
S     Sge    8.381968d*E (JD2406600 - 18000); since
S     Sge    JD2418000 - see Table.
U     Sge    VB A (B 9.6m, 92.0", 318deg). Min II 6.71;
U     Sge    0.014P <= dI <= 0.024P. In the region of the open cluster
U     Sge    Col 399. Not a member of the cluster. P var [06224, 08608].
U     Sge    Mean elements are given in the Table representing
U     Sge    epochs of Min within  +-0.008P. The shape of the light
U     Sge    curve varies.
V     Sge    VB A (B 13.9m, 9.7", 267deg); SB2 (K1 = 320 km/s,
V     Sge    K2 = 85 km/s). P var? The depth of eclipses
V     Sge    varies from 0.6m to 1.3m. The mean brightness outside
V     Sge    eclipses varies. There are also flares with amplitudes up
V     Sge    to 3m and small light variations with a time
V     Sge    scale of minutes, dozens of minutes and a few days.
V     Sge    spectrum description [03593, 09472].
X     Sge    VB A (B 13.18m, 6", 248deg).
Z     Sge    V1 (NGC 6838, M71). Globular cluster member. P var.
Z     Sge    Max = 2437870 + 175.3d*E (JD2437000 - 38700); since
Z     Sge    JD2438700 - see Table.
RS    Sge    The mean brightnese varies: Max = 2435999 + 1124d*E [08104].
RS    Sge    Two Algol-like light weakenings were also
RS    Sge    observed: JD2444837.22, 2444865.17 [09727].
RW    Sge    P var. according to [01363] Max = 2424289 + 429d*E. Since
RW    Sge    JD2434000 - see Table.
RZ    Sge    Porb ~97m [09771]. Mean cycle is given according to [09785].
RZ    Sge    Supermaxima are repeated with the cycle 266d. The period
RZ    Sge    of superhumps decreases from 101.3m till 100.8m.
SY    Sge    Min II 10.7. P var. Elements given in the Table are valid
SY    Sge    in the interval JD2425800 - 38300.
TU    Sge    d = 0.035P.
TX    Sge    P var. Max = 2425002 + 155.0d*E (JD2414900 - 25100);
TX    Sge    since JD2425000 - see Table.
UU    Sge    VB A (B 16.5m B, 4", 90deg). The nucleus of the planetary
UU    Sge    nebula Abell 63. Min II 14.41; d = 0.019P.
UU    Sge    The range of the combined light variation is given.
UU    Sge    The actual depth of Min I is about 4.3m. Large reflection
UU    Sge    effect.
UZ    Sge    Min II 11.6:. P var. Min I = 2429961.231 + 2.215750d*E
UZ    Sge    (JD2429000 - 41600); since JD2441600 - see Table.
VZ    Sge    VB A (B 12m, 28.2", 206deg).
WY    Sge    Nova Sge 1783 (Max JD2372494:). Min I = 2445137.8993 +
WY    Sge    0.1536342d*E; D = 0.16P. Brightness outside eclipses is
WY    Sge    usually ~18.7m, the depth of the eclipses is ~ 1.5 - 2m.
WY    Sge    At present outbursts by 1.6m are sometimes observed
WY    Sge    similar to the UG type variable outbursts, as well as
WY    Sge    rapid flickering of light [09708].
WZ    Sge    Nova Sge 1913, 1946, 1978. VB A (B 15.76m B, 7", 280deg).
WZ    Sge    Really it is not a nova. Three outbursts were registered
WZ    Sge    up to day: JD2420094, 32001, 43844 [09710, 09711].
WZ    Sge    There are superhumps on the light curve during the
WZ    Sge    outburst with 0.057250d >= P >= 0.05714d (A=0.3m V)
WZ    Sge    [09710, 09776]. There are light variations between
WZ    Sge    the outbursts (A = 0.14m - 0.3m). During some of light
WZ    Sge    weakenings Algol-like eclipses are observed (A = 0.2m)
WZ    Sge    with the elements: Min I = 2437547.72845 + 0.0566878455d*E
WZ    Sge    [09774]; D = 0.04P. d = 0.02P. There are also rapid light
WZ    Sge    oscillations (A <= 0.01m). The periods of these
WZ    Sge    oscillations before the 1978 outburst were 28.98s and
WZ    Sge    27.87s [09774], but after this outburst - 28.95963s [09775].
WZ    Sge    According to [09777], in 1976 - 78 these oscillations were
WZ    Sge    represented by the elements: Max = 2443311.790250 +
WZ    Sge    0.00032254826d*E + 9.8d*10**(-16)*E**2.
XY    Sge    According to [03705] the spectrum is earlier than M0.
AG    Sge    P = 117d?
BR    Sge    d = 0.030P.
CP    Sge    Min II 13.3.
CT    Sge    Multiple. The tabulated range is for combined magnitudes.
CU    Sge    Min II 11.3.
CW    Sge    Min II 11.7. P var? The shape of the light curve varies.
CZ    Sge    Min II 15.2.
DH    Sge    The shape of the light curve varies (1.1m <= A <= 1.7m).
DH    Sge    P var. Max = 2427612.509 + 0.4695844D*E (JD2427600 -
DH    Sge    38800) [04027]; since JD2438800 - see Table.
DH    Sge    Blazhko effect disappeared after the period change
DH    Sge    (A = 1.1m).
DI    Sge    P var. Max = 2427929 + 203.0d*E (JD2427500 - 30200)
DI    Sge    [02641]; since JD2437100 - see Table.
DK    Sge    Min II 13.0.
DL    Sge    Min II 11.5.
DM    Sge    Min II 11.6.
DP    Sge    P var. Max = 2427985.464 + 0.4883395d*E (JD2427985 - 33000);
DP    Sge    Max = 2432855.191 + 0.4883339d*E (JD2433000 - 40775);
DP    Sge    since JD2440775 - see Table.
DQ    Sge    Min II 14.8.
DS    Sge    Min II 16.0:.
DT    Sge    d = 0.05P:.
EH    Sge    VB A (B 15.6m).
EI    Sge    Min II 14.6.
ER    Sge    P var. Max = 2430515.460 + 0.4184209d*E
ER    Sge    (JD2427000 - 38400);
ER    Sge    Max = 2438443.388 + 0.4184356d*E (JD2438400 - 41800);
ER    Sge    since JD2441800 - see Table.
FF    Sge    d = 0.03P; Min II 13.0.
FG    Sge    VB A (B 14.2m, 8", 100deg). The central star of the
FG    Sge    planetry nebula PK 60deg (diameter 36", the age about 6000
FG    Sge    years). The brightness of the star steadily increased from
FG    Sge    13.6 pg in 1894 to the maximum in 1967, and then is
FG    Sge    steadily decreasing. In 1982 it was 11.0 B. In 1967 the
FG    Sge    strong absorption lines of rare earth elements appeared
FG    Sge    in the spectrum. The spectral class steadily becomes
FG    Sge    later. The signes of new planetary nebula ejection were
FG    Sge    observed. In 1962 the star entered the instability
FG    Sge    strip in the Mv, B-V diagram and began to pulsate
FG    Sge    with a small amplitude and increasing period: Min(V) =
FG    Sge    2442629 + 59.83d*E + 1.126d*E**2 (JD2442600 - 44530).
FG    Sge    In twenty years the period increased from 50d to 134d,
FG    Sge    the amplitude of pulsations changed from 0.2mV to 0.5mV;
FG    Sge    now it decreased again to 0.2mV, and the period is only
FG    Sge    90d [09780].
FH    Sge    Min II 13.5.
FL    Sge    There is a close companion 14m. In the minimum probably
FL    Sge    fainter than 15.9m.
FO    Sge    P var. Max = 2427578.0 + 67.8d*E (JD2427570 - 28120);
FO    Sge    Max = 2428134.4 + 72.7d*E (JD2428120 - 30150);
FO    Sge    since JD2430150 - see Table.
FP    Sge    Min II 14.9. P = 0.32100275d?
FT    Sge    P.K.55-1 deg 2. Not a planetary nebula.
FU    Sge    Min II 15.8.
FX    Sge    In the region of the globular cluster M71 (NGC 6838).
GI    Sge    Red.
GN    Sge    Min II 10.6.
GP    Sge    Red.
GY    Sge    P var. Max = 2431264.49 + 51.497d*E (JD2429490 - 34900)
GY    Sge    [07199]; Max = 2433787.42 + 51.5991d*E (JD2433600 - 37280),
GY    Sge    Max = 437911.04 + 51.2524d*E (JD2437280 - 40510) [06172];
GY    Sge    since JD2444450 - see Table.
HH    Sge    The cycles 23 - 26d and 300d are observed.
HM    Sge    VB A (B 14.20m, 10", 182deg). The brightness increased
HM    Sge    from 17.2m up to 11.3m pg in the interval JD2442280 -
HM    Sge    42650. Then the light variations in the infrared region
HM    Sge    appeared with P = 550d [09721, 09783] and A(K) = 1.5m.
HM    Sge    Radio and X-ray source.
IR    Sge    SF star in a close pair.
LN    Sge    SF star in a close pair.
MV    Sge    Possible member of the globular cluster Palomar 10.
MZ    Sge    Possible member of the globular cluster Palomar 10.
PT    Sge    P component of a close pair.
V0339 Sge    Extremely metal-weak.
V0366 Sge    O'Connell effect.
V0370 Sge    MinII - MinI = 0.38P.
V0378 Sge    VB A (B 13.7m, 20", 322deg, 2000).
V0380 Sge    VB AB (10.7m, 10.9m, 0.57", 74deg, 1990).
del   Sge    VB A (B, A = 0.04", P = 7 yr); SB2 (Porb = 3725d [09789]).
del   Sge    The last superior conjunction of the B-star and its
del   Sge    atmospheric eclipse was in March - April 1980 [09726].
R     Sgr    P var. Max = 2405776 + 271.0d*E (JD2399500 - 2407500);
R     Sgr    Max = 2407115 + 264.2d*E (JD2407100 - 9500);
R     Sgr    Max = 2418125 + 269.65d*E (JD2409500 - 19500);
R     Sgr    Max = 2433137 + 267.90d*E (JD2419500 - 36000);
R     Sgr    since JD2436000 - see Table.
S     Sgr    P var. Max = 2401029 + 230.6d*E (JD2401000 - 10000);
S     Sgr    Max = 2411638 + 229.2d*E (JD2410000 - 19500);
S     Sgr    Max = 2422222 + 232.81d*E (JD2419500 - 27000);
S     Sgr    since JD2427000 - see Table.
T     Sgr    Companion F3IV (ro < 0.8"). P var.
T     Sgr    Max = 2409013 + 385.1d*E (JD2401500 - 10500);
T     Sgr    Max = 2414582 + 399.0d*E (JD2413000 - 17500);
T     Sgr    Max = 2424363 + 387.9d*E (JD2417500 - 25500);
T     Sgr    since JD2425500 - see Table.
T     Sgr    S 5/6-e. There are Te lines and a very strong
T     Sgr    Li lambda 6708 line in the spectrum.
U     Sgr    The member of the open  cluster M25 (IC 4725).
U     Sgr    P var. Max = 2416628.046 + 6.744925d*E (JD2404480 - 30115)
U     Sgr    [00765]; since JD2430115 - see Table. [A/H] = 0.1.
W     Sgr    VB A (A 9.2m, 0.116", 153.3deg, 1976.477; B 13.5m, 33.4",
W     Sgr    233deg; C 13.5m, 47.9", 101deg). P var.
W     Sgr    Max = 2403198.39 + 7.594695d*E (JD2403100 - 34500); since
W     Sgr    JD2434500 - see Table.
X     Sgr    P var. Max = 2410006.22 + 7.01206d*E (JD2403000 - 17000);
X     Sgr    Max = 2424248.11 + 7.01245d*E (JD2417000 - 34500); since
X     Sgr    JD2434500 - see Table.
Y     Sgr    In the region of the open cluster M25 (IC 4725).
RR    Sgr    P var. Max = 2410008 + 336.0d*E (JD2410000 - 17100)
RR    Sgr    [09794]; Max = 2422755 + 332.73d*E (JD2422700 - 32100)
RR    Sgr    [00960]; since JD2432100 - see Table. OH, H2O emission.
RS    Sgr    VB A (B 9.65m V, 39.0", 86deg). Min II 6.28.
RT    Sgr    P var. Max = 2412759 + 303.1d*E (JD2412700 - 8300)
RT    Sgr    [00960]; Max = 2425588 + 308.8d*E (JD2422800 - 26700);
RT    Sgr    Max = 2428034 + 303.8d*E (JD2426700 - 33500);
RT    Sgr    since JD2433500 - see Table.
RU    Sgr    P var. Max = 2413062 + 242.3d*E (JD2410150 - 16700)
RU    Sgr    [00960]; Max = 2423670 + 242.3d*E (JD2422500 - 24500);
RU    Sgr    Max = 2428200 + 237.6d*E (JD2424500 - 28800); since
RU    Sgr    JD2428800 - see Table.
RV    Sgr    P var. Max = 2411206 + 319.3d*E (JD2410200 - 17000)
RV    Sgr    [00960]; Max = 2429032 + 321.3d*E (JD2422600 -
RV    Sgr    29500); since JD2429500 - see Table.
RW    Sgr    P var. Max = 2413798 + 189.0d*E (JD2413700 - 23000);
RW    Sgr    Max = 2431998 + 190.87d*E (JD2423000 - 33500);
RW    Sgr    since JD2433500 - see Table.
RX    Sgr    P var. Max = 2417730 + 330.3d*E (JD2413000 - 18500);
RX    Sgr    Max = 2420122 + 346d*E (JD2418500 - 20150);
RX    Sgr    Max = 2420122 + 323d*E (JD2420100 - 22200);
RX    Sgr    Max = 2424120 + 345d*E (JD2422200 - 24200);
RX    Sgr    Max = 2428785 + 332.2d*E (JD2424000 - 31500);
RX    Sgr    since JD2431500 - see Table.
RY    Sgr    VB A (B 15.69m, 12"). There are pulsational light
RY    Sgr    variations (0.1m < A < 1.5m) with the elements:
RY    Sgr    Max = 2433670 + 38.6056d*E - 78d*10**(-5)*E**2.
RY    Sgr    light curve [09798, 09799]; spectrum description [06261].
ST    Sgr    S 6/3-e.
SU    Sgr    VB A (B 13.5m, 1.0", 240deg, 1932.45).
SU    Sgr    earlier P = 88d was observed [00017].
SV    Sgr    In the nebula M8 (NGC 6523).
SW    Sgr    P var. Max = 2416338 + 290.3d*E (JD2414000 - 16500);
SW    Sgr    Max = 2428507 + 288.5d*E (JD2422500 - 29000);
SW    Sgr    Max = 2429088 + 293.5d*E (JD2429000 - 33000);
SW    Sgr    since JD2433000 - see Table.
SX    Sgr    Min II 9.62; d = 0.05P. P var. Min I = 2429114.249 +
SX    Sgr    4.15395762d*E (JD2410000 - 29150) [00007];
SX    Sgr    since JD2429000 - see Table.
SY    Sgr    In the region of the nebula S188.
SZ    Sgr    VB A (B 12.5m V, 2.0", 212deg.)
VV    Sgr    In the region of the open cluster NGC 6494. OH, H2O
VV    Sgr    emission.
VX    Sgr    P var; 1m <= A <= 6m. SIO, H2O, OH maser.
VX    Sgr    Light curve (1935-1969) [06615].
VY    Sgr    [A/H] = 0.5.
WX    Sgr    VB A (B 12.5m, 0.4", 88deg). P var. Min = 2419317.259 +
WX    Sgr    2.129095d*E (JD2419300 - 24700) [00457]; Min =
WX    Sgr    2424729.418 + 2.129113d*E (JD2424700 - 39700)
WX    Sgr    [00279]; since JD2440000 - see Table.
WY    Sgr    Min II 10.3.
WZ    Sgr    The member of the open cluster C 1814-190. [A/H] = 0.4.
XX    Sgr    P var. Max = 2419189.730 + 6.424264d*E (JD2419100 - 30100)
XX    Sgr    [00637]; since JD2435000 - see Table.
XZ    Sgr    Min II 8.95; d = 0.022P. P var. Min I = 2420311.519 +
XZ    Sgr    3.275537d*E (JD2420300 - 28000) [01604]; Min I =
XZ    Sgr    2436440.137 + 3.27549d*E (JD2428000 - 37500)
XZ    Sgr    [02516]; Min I = 2441150.348 + 3.2755357d*E
XZ    Sgr    (JD2437500 - 41500) [07084]; since JD2441500 - see Table.
YY    Sgr    Min II 10.64; Min II = 2433075.8296 + 2.628463d*E
YY    Sgr    [02302]. Apsidal motion period is about 300 years.
AL    Sgr    P var. Max = 2425792 + 79.07d*E (JD2421000 - 26000);
AL    Sgr    since JD2426000 - see Table.
AN    Sgr    P var. Max = 2425720 + 339.62d*E (JD2415000 - 26000);
AN    Sgr    Max = 2428360 + 330.0d*E (JD2426000 - 28500);
AN    Sgr    since JD2428500 - see Table.
AP    Sgr    SB? [09004].
AR    Sgr    There is a square term in the elements:
AR    Sgr    -[0.0031d (E-30)**2 + 8.8d].
AS    Sgr    Planetary nebula HB6 = 7 + 1deg 1.
AU    Sgr    In the region of the open cluster and the diffuse nebula
AU    Sgr    NGC 6514 (M20).
AV    Sgr    In the region of the open cluster NGC 6546. Not a member
AV    Sgr    of the cluster. [A/H] = 0.4. P var.
AV    Sgr    Max = 2429083.30 + 15.4093d*E (JD2421400 - 39100); since
AV    Sgr    JD2439100 - see Table.
AW    Sgr    VB A (B 16m, 15", 97deg).
AW    Sgr    In the region of the open cluster NGC 6546.
AY    Sgr    [A/H] = 0.2.
BB    Sgr    VB A (B = V4088 Sgr, 7.49m - 7.87m, 93.5", 102deg).
BB    Sgr    In the region of the open cluster Cr394.
BE    Sgr    A var (0.6m <= A <= 1.1m).
BM    Sgr    P var.
BN    Sgr    Min II 9.37; d = 0.04P:.
BN    Sgr    Soft X-ray source. P var [01600].
BQ    Sgr    d = 0.017P. P var. Min = 2412592.7905 + 8.01964d*E
BQ    Sgr    (JD2412590 - 22220) [01696]; since JD2422220 - see Table.
CC    Sgr    In the region of the globular cluster NGC 6723.
CD    Sgr    In the region of the globular cluster NGC 6723. P var.
CD    Sgr    Max = 2416247 + 266.62d*E
CD    Sgr    (JD2411000 - 23000); since JD2423000 - see Table.
CE    Sgr    In the region of the globular cluster NGC 6723.
CE    Sgr    SF component of a close double.
CF    Sgr    In the region of the globular cluster NGC 6723.
CF    Sgr    P var. Max = 2415632.81 + 0.570026d*E (JD2411000 -
CF    Sgr    23800) [01616]; since JD2423900 - see Table.
CG    Sgr    In the region of the globular cluster NGC 6723.
DH    Sgr    In the region of the globular cluster NGC 6809 (M55).
DI    Sgr    In the region of the globular cluster NGC 6809 (M55).
DK    Sgr    In the region of the globular cluster NGC 6809 (M55).
DM    Sgr    In the region of the globular cluster NGC 6809 (M55).
DO    Sgr    In the region of the globular cluster NGC 6809 (M55).
DP    Sgr    In the region of the globular cluster NGC 6809 (M55).
DR    Sgr    In the region of the globular cluster NGC 6809 (M55).
DS    Sgr    In the region of the globular cluster NGC 6809 (M55).
DV    Sgr    d = 0.044P.
EG    Sgr    d = 0.010P.
FV    Sgr    P var. Max = 2424010 + 269.5d*E (JD2424000 - 27500)
FV    Sgr    [00251]; since JD2427500 - see Table.
GG    Sgr    P var. Max = 2413840 + 286.5d*E (JD2413800 - 24000);
GG    Sgr    since JD2424000 - see Table.
GK    Sgr    According to [05869] - eclipsing.
GU    Sgr    There are also light variations with P = 37.5d,
GU    Sgr    0.4m <= A(V) <= 1.5m [06273].
HH    Sgr    VB (ro = 0.1').
IR    Sgr    VB B (A 13.6m; B 10", 220deg).
KO    Sgr    Similar to UG. It is possible that the observations in Min
KO    Sgr    brightness refer to a companion.
LN    Sgr    P = 227.0d?
LZ    Sgr    VB A (B 16m, 7", 30deg).
MV    Sgr    Very hot hydrogen deficient extreme helium carbon star.
MW    Sgr    P var. Max = 2418940 + 202.3d*E (JD2418900 - 23900);
MW    Sgr    Max = 2428753 + 206.5d*E (JD2423900 - 28950);
MW    Sgr    since JD2428950 - see Table.
NP    Sgr    The cycles 100 - 300d are possible.
OW    Sgr    In the region of the open cluster NGC 6716.
V0348 Sgr    VB A (B 15m pg, 16", 73deg). Very hot hydrogen deficient
V0348 Sgr    helium carbon star.
V0348 Sgr    By the character of light variation and the spectrum the
V0348 Sgr    star is unique. The light curve resembling those of RCB
V0348 Sgr    type stars is superimposed by conspicuons irregular and
V0348 Sgr    semiregular variations with the mean cycle about 200d
V0348 Sgr    [02449, 09824]. The star is surrounded by a nebula the
V0348 Sgr    radius of which equals 1". A fainter nebulous envelope is
V0348 Sgr    observed up to 7" from the star. Large infrared
V0348 Sgr    excess. Spectrum description [02451, 09825]. Probably
V0348 Sgr    the star is intermediate between the RCB variables
V0348 Sgr    And planetary nebula Wolf-Rayet central stars.
V0350 Sgr    SB [09004].
V0354 Sgr    d = 0.02P.
V0356 Sgr    Min II 7.24; DII = 0.20P:; d = 0.05P;
V0356 Sgr    0.490P (1928) <= Min II - Min I <= 0.505P (1951).
V0356 Sgr    Apsidal motion is possible.
V0366 Sgr    P var. Max = 2425479.448 + 0.4779616d*E (JD2423990 - 28780)
V0366 Sgr    [00705]; since JD2435600 - see Table. [Ca/H] = -0.73.
V0367 Sgr    [Ca/H] = -1.21.
V0377 Sgr    The epoch of light min is given in the Table.
V0377 Sgr    P var. Min = 2426071.24 + 16.17076d*E (JD2425300 - 26600)
V0377 Sgr    [00048]; Min = 2427350.25 + 16.19326d*E (JD2426600 - 28700)
V0377 Sgr    [01400]; Min = 2436358.98 + 16.1575d*E
V0377 Sgr    (JD2436200 - 37300); Min = 2437863.09 + 16.1925d*E
V0377 Sgr    (JD2437660 - 39100); Min = 2440114.81 + 16.2407d*E
V0377 Sgr    (JD2440200 - 560); since JD2440950 - see Table.
V0397 Sgr    There is a square term in the elements:
V0397 Sgr    -0.009d*10**(-6)*E**2
V0401 Sgr    Min II 14.1.
V0403 Sgr    There is a nonlinear term in the elements:
V0403 Sgr    -0.013d*10**(-6)*E**2.
V0410 Sgr    VB A (B 13.6m, 270deg).
V0426 Sgr    Min II 13.3.
V0427 Sgr    There is a nonlinear term in the elements:
V0427 Sgr    -131d*10**(-10)*E**2. The shape of the light curve varies:
V0427 Sgr    0.17P <= M - m <= 0.22P.
V0431 Sgr    Min II 14.9.
V0437 Sgr    Min II 14.0.
V0440 Sgr    Delta(S) = 9. P var. P = 0.4774659d (JD2416000 - 23000)
V0440 Sgr    [00752]; P < 0.4774659d (JD2422000 - 26000) [00235];
V0440 Sgr    Max = 2426581.203 + 0.477474d*E (JD2426000 - 29460) [01000];
V0440 Sgr    since JD2437100 - see Table.
V0453 Sgr    There is a nonlinear term in the elements:
V0453 Sgr    +0.003d*10**(-6)*E**2.
V0457 Sgr    There is a nonlinear term in the elements:
V0457 Sgr    -0.005d*10**(-6)*E**2.
V0466 Sgr    There is a nonlinear term in the elements:
V0466 Sgr    +0.03d*10**(-6)*E**2.
V0496 Sgr    Min II 14.3.
V0497 Sgr    Min II 16.0.
V0505 Sgr    Min II 6.63. P var. Min I = 2433515.3295 + 1.18287141d*E
V0505 Sgr    (JD2425500 - 35800) [01642]; Min I = 2437494.4964 +
V0505 Sgr    1.1828622d*E (JD2435800 - 37500); Min I =
V0505 Sgr    2440055.3991 + 1.1828650d*E (JD2437500 - 40100);
V0505 Sgr    Min I = 2442656.5283 + 1.18286917d*E (JD2440100 -
V0505 Sgr    42670); since JD2442670 - see Table. The shape of the
V0505 Sgr    light curve varies. Deviations from the mean light curve
V0505 Sgr    vary with P = 310d. The difference of Min I and Min II
V0505 Sgr    depths varies by 0.05m [09830].
V0511 Sgr    P var. Max = 2423950 + 158.8d*E (JD2411300 - 23950);
V0511 Sgr    since JD2423950 - see Table.
V0515 Sgr    There is a nonlinear term in the elements: +0.015d*E**2.
V0519 Sgr    There is a nonlinear term in the elements: +0.0046d*E**2.
V0520 Sgr    There is a nonlinear term in the elements: +0.051d*E**2.
V0523 Sgr    Min II 9.88. Apsidal motion is observed. In the Table the
V0523 Sgr    epoch of Min I is given corresponding to the moment of
V0523 Sgr    line of apsides coinciding with the line of sight, when
V0523 Sgr    Min II - Min I = 0.50P. The mean period according to
V0523 Sgr    [02453] is given; with this period O - C deviations do not
V0523 Sgr    exceed  +-0.06P for both minima. The period of apsidal
V0523 Sgr    motion is 248 years [02453]. Min II - Min I = 0.39P in 1953.
V0524 Sgr    Min II 11.2.
V0525 Sgr    Min II 8.51.
V0526 Sgr    VB A (B 12.40m, 8.6", 7.3deg). Min II 10.20, DII = 0.17P;
V0526 Sgr    dI = 0.006P, dII = 0.013P.
V0526 Sgr    There are periodic terms in the elements:
V0526 Sgr    +0.1369d*sin(0.01295deg*E) - 0.0115d*sin(0.0259deg*E) +
V0526 Sgr    0.0011d*sin(0.0388deg*E). Min II = 2422055.0453 +
V0526 Sgr    1.919411d*E - 0.1369d*sin(0.01295deg*E) -
V0526 Sgr    0.0115d*sin(0.0259deg*E) - 0.0011d*sin(0.0388deg*E).
V0526 Sgr    The period of apsidal motion is 146 years. e = 0.224.
V0527 Sgr    P var. Max = 2426904.95 + 1.258956d*E (JD2425790 - 7650)
V0527 Sgr    [01648]; since JD2438200 - see Table.
V0551 Sgr    VB B (A 16.5m; B 12", 135deg).
V0552 Sgr    P var. The elements given in the Table are
V0552 Sgr    valid since JD2418400.
V0554 Sgr    Min II 14.5.
V0557 Sgr    P var. Max = 2415110.5 + 16.233d*E (JD2415100 - 22000);
V0557 Sgr    Max = 2426100.0 + 16.260d*E (JD2423900 - 27700) [00251];
V0557 Sgr    Max = 2428097.70 + 16.171d*E (JD2427700 - 28800) [00296];
V0557 Sgr    since JD2428800 - see Table.
V0558 Sgr    Min II 14.3.
V0564 Sgr    P var. Max = 2424056 + 27.8d*E (JD2423780 - 26000)
V0564 Sgr    [00251]; Max = 2428403.3 + 27.99d*E (JD2427870 - 29160)
V0564 Sgr    [00296]; Max = 2429158.2 + 27.2d (JD2429150 - 515);
V0564 Sgr    since JD2429515 - see Table.
V0567 Sgr    The central star of the planetary nebula P.K.355 -6deg 1
V0567 Sgr    (M3-21).
V0573 Sgr    Min II 12.7.
V0574 Sgr    Min II 14.7.
V0578 Sgr    According to [02448], Max = 2428710 + 253d*E.
V0593 Sgr    P var. Max = 2414150 + 230d*E (JD2414100 - 22900);
V0593 Sgr    since JD2423900 - see Table.
V0598 Sgr    d = 0.05P.
V0611 Sgr    P var. Max = 2414150 + 123d*E (JD2414150 - 19000);
V0611 Sgr    since JD2420250 - see Table.
V0611 Sgr    The period must probably be doubled because the star
V0611 Sgr    resembles RV Tau (Min II 16.2).
V0612 Sgr    P var. Max = 2413750 + 107.9d*E (JD2413700 - 17900);
V0612 Sgr    since JD2418800 - see Table.
V0615 Sgr    P.K.356 -7deg 1 = He 2-349.
V0626 Sgr    P var? Max = 2427715.4 + 26.745d*E (JD2425380 - 28800)
V0626 Sgr    [00046]; since JD2434500 - see Table.
V0631 Sgr    Min II 14.2.
V0632 Sgr    P var. Max = 2413350 + 263d*E (JD2413300 - 19000);
V0632 Sgr    since JD2420200 - see Table.
V0633 Sgr    P var. Max = 2415110 + 224d:*E (JD2415000 - 18800);
V0633 Sgr    since JD2420000 - see Table.
V0638 Sgr    P var? Max = 2412670 + 73.1d*E (JD2412600 - 14540);
V0638 Sgr    since JD2414800 - see Table.
V0646 Sgr    P var. Max = 2413350 + 95d*E (JD2413300 - 15900);
V0646 Sgr    since JD2423900 - see Table.
V0655 Sgr    P = 213.0d? The coordinates given in [05869] are erroneous.
V0660 Sgr    P var. Max = 2426460 + 235.6d*E (JD2426400 - 35700)
V0660 Sgr    [00251]; since JD2435600 - see Table.
V0663 Sgr    P var. Max = 2426160 + 305d*E [00251];
V0663 Sgr    since JD2435600 - see Table.
V0671 Sgr    P = 292.5d?
V0672 Sgr    P var? Max = 2424680 + 228d*E [00251]; since
V0672 Sgr    JD2435600 - see Table.
V0674 Sgr    P var. Max = 2425830 + 249d*E [00251]; since
V0674 Sgr    JD2435600 - see Table.
V0675 Sgr    (k - b)2 = -0.01; Delta(S) = 11.
V0676 Sgr    P var. Max = 2414140 + 181d*E (JD2414100 - 22600)
V0676 Sgr    [00251]; since JD2423900 - see Table.
V0679 Sgr    P var. Max = 2415900 + 225d*E (JD2415900 - 22200)
V0679 Sgr    [00251]; Max = 2425440 + 223.1d*E (JD2425000 - 29000);
V0679 Sgr    since JD2429000 - see Table.
V0683 Sgr    Min II 12.5.
V0686 Sgr    P var? Max = 2425390 + 225.3d*E [00251]; since
V0686 Sgr    JD2435600 - see Table.
V0687 Sgr    Min II 12.2.
V0691 Sgr    P var? Max = 2426095.550 + 0.46911d*E [00251];
V0691 Sgr    since JD2435630 - see Table.
V0703 Sgr    Var 4. According to [02951] the range of light variation,
V0703 Sgr    the type of variability and the elements of light
V0703 Sgr    variation are erroneously assigned in [01640] to the star
V0703 Sgr    Var 3.
V0705 Sgr    Min II 12.9.
V0710 Sgr    P var. Min = 2426101.550 + 2.3817d*E [00251]; Min =
V0710 Sgr    2431286.425 + 2.381633d*E (JD2428390 - 35700) [03513].
V0713 Sgr    P var? Max = 2424680 + 253.4d*E [00251]; since
V0713 Sgr    JD2435600 - see Table.
V0716 Sgr    P var? Max = 2424670 + 277d*E [00251]; since
V0716 Sgr    JD2435600 - see Table.
V0718 Sgr    P var? Max = 2425850 + 153.2d*E [00251]; since
V0718 Sgr    JD2435600 - see Table.
V0721 Sgr    P = 71:d?
V0725 Sgr    Unique star.
V0725 Sgr    The mean brightness increased from 13.0m to 12.4m
V0725 Sgr    since 1889 to 1915, and fell to 12.8m in 1926. From
V0725 Sgr    1895 to 1926 real shortperiodic oscillations with the
V0725 Sgr    amplitude about 0.4m. In 1928 the amplitude suddenly
V0725 Sgr    increased by almost 2m, but the magnitude in maximum
V0725 Sgr    remained unchanged. From 1928 to 1935 the light
V0725 Sgr    variations became periodic, the period increasing every
V0725 Sgr    year by 1d in accordance with the formula:
V0725 Sgr    Min = 2426087 + 15.933d*E + 0.0233d*E**2.
V0725 Sgr    In 1935 P = 21d. Since 1936 only small oscillations of
V0725 Sgr    brightness with a gradual increase of the mean magnitude
V0725 Sgr    from 14.3m to 13.9m B (1969). Photoelectric observations
V0725 Sgr    in 1968 - 69 reveal the light variations 12.33m - 12.72m V
V0725 Sgr    with possible periods 15.4d in 1968 and 45.3d in 1969. In
V0725 Sgr    1973 12.28m - 12.58m V, B-V = +1.37, P = 50d [07101].
V0727 Sgr    VB A (B = V728 Sgr, 14.7m - 15.9m, 25", 108deg).
V0728 Sgr    VB B (A = V727 Sgr, B 25", 108deg).
V0734 Sgr    Min II 13.1.
V0735 Sgr    VB A (B 15.5m, 6", 315deg). According to B-V, U-B values
V0735 Sgr    and spectrum the star is not a UG type variable [09840].
V0738 Sgr    In the region of the globular cluster NGC 6558.
V0738 Sgr    According to [05403], RV? P = 86.78d?
V0743 Sgr    Min II 14.2.
V0745 Sgr    P var. Max = 2416560 + 385.1d*E (JD2411000 - 19260);
V0745 Sgr    since JD2419260 - see Table.
V0748 Sgr    Min II 14.7; d = 0.04P.
V0750 Sgr    d = 0.02P:.
V0752 Sgr    Min II 12.7.
V0755 Sgr    d = 0.01P.
V0757 Sgr    Min II 13.8; d = 0.06P.
V0760 Sgr    Min II 13.4. P var. Min = 2414059.5 + 45.10d*E
V0760 Sgr    (JD2412800 - 19000); since JD2419000 - see Table.
V0761 Sgr    Min II 12.8; d = 0.05P.
V0762 Sgr    P var. Max = 2414100 + 461d*E (JD2411000 - 22860);
V0762 Sgr    since JD2422860 - see Table.
V0763 Sgr    P var. The observations are satisfied by the given
V0763 Sgr    elements since JD2415000.
V0766 Sgr    d = 0.05P.
V0768 Sgr    Min II 13.0.
V0770 Sgr    Min II 13.1.
V0773 Sgr    [A/H] = 0.1.
V0777 Sgr    d = 0.055P.
V0778 Sgr    Min II 12.1.
V0779 Sgr    Min II 12.0.
V0780 Sgr    Min II 12.9; d = 0.08P.
V0782 Sgr    d = 0.045P.
V0784 Sgr    Min II 12.8.
V0786 Sgr    d = 0.025P.
V0789 Sgr    In the region of the open cluster Tr 31.
V0789 Sgr    P = 5.10470d (Min II 12.7)? [00478].
V0791 Sgr    d = 0.03P:.
V0792 Sgr    Min II 12.2. In the region of the open cluster
V0792 Sgr    and the diffuse nebula NGC 6514 (M 20).
V0793 Sgr    P var. Max = 2412610 + 195d*E (JD2412600 - 19400);
V0793 Sgr    since JD2423400 - see Table.
V0794 Sgr    P var. Min I = 2413723 + 173.48d*E (JD2413700 -
V0794 Sgr    23750); since JD2423750 - see Table.
V0801 Sgr    Min II 14.9.
V0802 Sgr    [A/H] = -0.4.
V0803 Sgr    P = 3.771748d?
V0818 Sgr    The shape of the light curve varies.
V0819 Sgr    P var?
V0824 Sgr    Min II 15.2.
V0828 Sgr    There is a close companion.
V0838 Sgr    P var?
V0839 Sgr    P var? Max = 2426170.126 + 1.835347d*E (JD2425700 - 26600)
V0839 Sgr    [01598]; since JD2441500 - see Table.
V0841 Sgr    The shape of the light curve varies.
V0844 Sgr    P var?
V0845 Sgr    Min II 14.6.
V0859 Sgr    The shape of the light curve varies.
V0879 Sgr    There is a close companion.
V0882 Sgr    Min II 14.6.
V0884 Sgr    0.20P <= M - m <= 0.40P. Blazhko effect.
V0889 Sgr    0.14P <= M - m <= 0.24P. Blazhko effect.
V0902 Sgr    Min II 14.8.
V0903 Sgr    Min II 13.0.
V0919 Sgr    Spectrum description [09845].
V0935 Sgr    P var. Max = 2420040 + 232.0d*E (JD2419500 - 28650);
V0935 Sgr    since JD2428600 - see Table.
V0938 Sgr    P = 138.27d?
V0960 Sgr    nP = 1734d.
V0966 Sgr    Min II 14.0.
V0977 Sgr    d = 0.03P.
V0981 Sgr    Min II 14.8.
V0985 Sgr    Min II 14.3.
V0986 Sgr    d = 0.015P.
V0993 Sgr    dI = 0.05P:; Min II 13.7, DII = 0.09P, dII = 0.00P.
V0994 Sgr    Min II 12.8:.
V0998 Sgr    The depth of Min II 0.04m:.
V1000 Sgr    Min II 13.9.
V1002 Sgr    Min II 13.7.
V1004 Sgr    [A/H] = -0.2.
V1005 Sgr    Min II 13.9.
V1013 Sgr    Min II 15.0.
V1017 Sgr    VB B (A 10.6m V; B 15", 270deg).
V1017 Sgr    For a long time the star was considered to be a recurrent
V1017 Sgr    nova. Three considerable flares were observed: in 1901
V1017 Sgr    (10.8m), 1919 (6.2m), and 1973 (10.5m). Composite spectrum
V1017 Sgr    with a trace of a hot component [03872].
V1023 Sgr    In the region of the open cluster Cr 394. Min II 13.0:.
V1026 Sgr    Min II 13.4.
V1028 Sgr    Min II 14.4.
V1032 Sgr    Min II 15.0.
V1033 Sgr    The shape of the light curve varies. Blazhko effect?
V1034 Sgr    d = 0.025P:.
V1056 Sgr    Min II 14.1.
V1063 Sgr    The shape of the light curve strongly varies. Blazhko
V1063 Sgr    effect?
V1068 Sgr    Min II 15.4.
V1069 Sgr    The shape of the light curve strongly varies. Blazhko
V1069 Sgr    effect?
V1071 Sgr    P = 1.3560996d?
V1072 Sgr    The shape of the light curve strongly varies. Blazhko
V1072 Sgr    effect?
V1080 Sgr    P var. The shape of the light curve varies.
V1081 Sgr    P var?
V1089 Sgr    Cycle <= 30d.
V1100 Sgr    d = 0.02P:.
V1108 Sgr    Min II 11.9; Min II - Min I = 0.516P.
V1109 Sgr    Min II 14.5.
V1127 Sgr    There is a nonlinear term in the elements:
V1127 Sgr    +78.10d**(-10)*E**2.
V1136 Sgr    d = 0.020P.
V1148 Sgr    In the region of the globular cluster NGC 6553.
V1153 Sgr    P var? Max = 2428391.266 + 1.332624d*E (JD2427680 -
V1153 Sgr    30910); since JD2435630 - see Table.
V1177 Sgr    Min II 11.4.
V1178 Sgr    d = 0.03P:.
V1180 Sgr    [A/H] = -0.4.
V1181 Sgr    [A/H] = 0.6. P var. Max = 2428452.25 + 21.341d*E
V1181 Sgr    (JD2427400 - 31000) [01638]; since JD2433000 - see Table.
V1185 Sgr    [A/H] = -0.5. P var. Max = 2428778.86 + 13.9123d*E
V1185 Sgr    (JD2427500 - 32750) [01638]; Max = 2437485.4 +
V1185 Sgr    13.901345d*E (JD2437100 - 43760) [08519];
V1185 Sgr    since JD2444000 - see Table.
V1187 Sgr    [A/H] = -0.8.
V1188 Sgr    [CA/H] = -0.37.
V1189 Sgr    [A/H] = -1.1.
V1190 Sgr    P = 3.000078d?
V1191 Sgr    Min II 14.4.
V1205 Sgr    The alternative period is possible: 0.659820d [01638].
V1209 Sgr    A var.
V1211 Sgr    Delta(S) = 3:.
V1214 Sgr    There is a nonlinear term in the elements:
V1214 Sgr    -0.25d*10**(-7)*E**2.
V1216 Sgr    mu = 0.720", P = 106.7deg.
V1223 Sgr    As a rule has a persistent high state; five drops by two
V1223 Sgr    to more than three magnitudes have been registered and a
V1223 Sgr    twelve year interval of irregular variations at
V1223 Sgr    intermediate magnitudes. According to [09850] there are
V1223 Sgr    slow variations in brightness by 0.15m on a time scale
V1223 Sgr    of ~1 day. They are superimposed by variations with the
V1223 Sgr    orbital period P orb (Max = 2444749.9866 + 0.140239d*E)
V1223 Sgr    and with amplitude up to 0.15m. These variations in their
V1223 Sgr    turn are superimposed by the others: with P = 794.38s
V1223 Sgr    and the amplitude from 0.03m up to 0.15m
V1223 Sgr    (Max = 2444750.00404 + 0.009194215d*E and (sometimes) with
V1223 Sgr    P = 849.8s and a twice smaller amplitude
V1223 Sgr    (Max = 2444750.00350 + 0.00983588d*E). Besides there are
V1223 Sgr    rapid brightness variations on time scales 10 - 100s by
V1223 Sgr    0.10m - 0.20m, and high frequency flickering by 0.05m.
V1223 Sgr    According to [09851], the period of X-ray pulses associated
V1223 Sgr    with the rotation of the compact object is 12.5 minutes.
V1276 Sgr    Min II 14.3.
V1280 Sgr    Brightness of Max varies by 2m with the period 5230d.
V1281 Sgr    The light variation is not strictly periodic.
V1282 Sgr    P var. Min = 2427651.297 + 1.754574d*E (JD2427650 -
V1282 Sgr    30560) [00705]; since JD2435600 - see Table.
V1284 Sgr    Min II 13.5. EB?
V1287 Sgr    Var 3. According to [02951] the range of light variation of
V1287 Sgr    Var 4 (V703 Sgr), the type of variability and the elements
V1287 Sgr    of light variation of Var 4 (V703) are erroneously
V1287 Sgr    assigned in [01640] to the star Var 3.
V1287 Sgr    According to [02951] the range of light variation, the type
V1287 Sgr    of variability and the elements of light variation are
V1287 Sgr    erroneously assigned in [01640] to the star Var 4.
V1287 Sgr    Min II 14.8.
V1290 Sgr    [A/H] = -1.2.
V1303 Sgr    [A/H] = -0.8. P var? Max = 2438241.176 + 18.46812d*E
V1303 Sgr    (JD2427700 - 38250) [00001]; since JD2444000 - see Table.
V1304 Sgr    [A/H] = 0.3. P var. Max = 2428758.10 + 12.9287d*E
V1304 Sgr    (JD2427590 - 28820) [01640]; since JD2435600 - see Table.
V1309 Sgr    Not far from V4032 Sgr.
V1311 Sgr    V 14 in the globular cluster NGC 6656 (M22).
V1311 Sgr    Not a member of the cluster.
V1312 Sgr    P var? Max = 2428815.600 + 0.6011427d*E (JD2427590 - 28820)
V1312 Sgr    [01640]; since JD2435630 - see Table.
V1314 Sgr    P var? Max = 2428346.536 + 0.657489d*E (JD2427600 -
V1314 Sgr    28820) [01640]; since JD2435630 - see Table.
V1317 Sgr    P var?
V1327 Sgr    SR?, L? [08424].
V1328 Sgr    P = 0.39937d?
V1329 Sgr    VB B (A 17.2m; B 1.4", 120deg). P var. Max = 2432388.777 +
V1329 Sgr    0.48306d*E (JD2431670 - 32740) [03524];
V1329 Sgr    since JD2443300 - see Table.
V1331 Sgr    Min II 16.5.
V1352 Sgr    P var. Max = 2431998.851 + 0.49505d*E (JD2431670 -
V1352 Sgr    33150) [01680]; Max = 2443341.844 + 0.49493d*E
V1352 Sgr    (JD2443300 - 350); Max = 2444087.558 + 0.49516d*E
V1352 Sgr    (JD2444050 - 110); in the interval JD2444400 - 410 - see
V1352 Sgr    Table.
V1356 Sgr    Min II 18.0:.
V1357 Sgr    Min II 19.0.
V1359 Sgr    P var?
V1369 Sgr    P var. Max = 2432736.821 + 0.52956d*E (JD2431670 - 33150)
V1369 Sgr    [03524]; since JD2440700 - see Table.
V1374 Sgr    Delta(S) = 1.
V1378 Sgr    Delta(S) = -3:.
V1387 Sgr    Delta(S) = 3.
V1389 Sgr    The epoch of Min brightness is given.
V1390 Sgr    Min II 17.6.
V1392 Sgr    P var. Max = 2432739.791 + 0.55032d*E (JD2431670 - 33150)
V1392 Sgr    [03524]; since JD2440700 - see Table.
V1393 Sgr    Delta(S) = 3.
V1394 Sgr    Min II 18.0.
V1401 Sgr    The epoch of Min brightness is given.
V1405 Sgr    P var. Max = 2432031.778 + 0.46511d*E (JD2431670 - 33150)
V1405 Sgr    [06094]; since JD2443300 - see Table.
V1408 Sgr    A var (0.5m <= A <= 1.4m).
V1409 Sgr    P var. Max = 2432739.822 + 0.65159d*E (JD2431670 - 33150)
V1409 Sgr    [03524]; since JD2443300 - see Table.
V1412 Sgr    The epoch of Min brightness is given.
V1415 Sgr    P var?
V1416 Sgr    Delta(S) = 3. P var? Max = 2432002.875 + 0.42767d*E
V1416 Sgr    (JD2431670 - 33150) [06094]; since JD2440700 - see Table.
V1418 Sgr    P var. Max = 2432740.818 + 0.45423d*E (JD2431670 - 33150)
V1418 Sgr    [03524]; since JD2440700 - see Table.
V1419 Sgr    P var. Max = 2432061.669 + 0.57144d*E (JD2431670 - 33150)
V1419 Sgr    [01680]; since JD2440700 - see Table.
V1425 Sgr    Min II 18.8.
V1426 Sgr    Delta(S) = 1.5.
V1429 Sgr    The epoch of Min brightness is given.
V1435 Sgr    Min II 18.0; Min II - Min I = 0.53P.
V1437 Sgr    V8 (NGC 6522); not a member of the globular cluster.
V1438 Sgr    V9 (NGC 6522); not a member of the globular cluster.
V1439 Sgr    P = 0.53711d? [06094].
V1443 Sgr    Min II 18.6.
V1446 Sgr    Min II 18.0.
V1447 Sgr    Min II 18.2.
V1454 Sgr    Min II 15.4.
V1457 Sgr    Min II 19.0.
V1459 Sgr    The depth of Min II is 0.04m.
V1460 Sgr    P var. Max = 2432067 + 162.0d*E (JD2431670 - 33150)
V1460 Sgr    [01680]; since JD2440340 - see Table.
V1464 Sgr    Delta(S) = 1.
V1465 Sgr    P var. Max = 2431702.660 + 0.45757d*E (JD2431700 - 940);
V1465 Sgr    Max = 2432706.945 + 0.45757d*E (JD2431940 - 32740) [03524];
V1465 Sgr    since JD2440740 - see Table.
V1466 Sgr    The epoch of Min brightness is given.
V1473 Sgr    According to [08424] P = 340d.
V1487 Sgr    Min II 18.8.
V1491 Sgr    Min II 18.5.
V1498 Sgr    SP component of a close pair. P var.
V1498 Sgr    Max = 2432739.728 + 0.47467d*E (JD2431670 - 33150) [06094];
V1498 Sgr    since JD2443300 - see Table.
V1508 Sgr    VB.
V1509 Sgr    Min II 18.1:.
V1510 Sgr    According to [06094], P = 0.48546d.
V1516 Sgr    P var? Max = 2432740.753 + 0.49709d*E (JD2431670 -
V1516 Sgr    33150) [03524]; since JD2440700 - see Table.
V1517 Sgr    P < 2.0d.
V1523 Sgr    P var? Max = 2432417.702 + 0.36202d*E (JD2431670 - 33150)
V1523 Sgr    [03524]; since JD2443300 - see Table.
V1526 Sgr    Min II 18.3.
V1537 Sgr    Min II 17.4; Min II - Min I = 0.54P.
V1540 Sgr    According to [08424], P = 465d.
V1546 Sgr    The epoch of Min brightness is given.
V1550 Sgr    P = 0.37432d? [06094].
V1554 Sgr    Min II 17.5.
V1557 Sgr    Delta(S) = 8.
V1558 Sgr    Delta(S) = 1.
V1559 Sgr    The depth of MinII is 0.04m.
V1561 Sgr    Min II 17.7.
V1567 Sgr    Min II 18.0.
V1569 Sgr    Min II 18.6.
V1576 Sgr    [Ca/H] = -1.23.
V1577 Sgr    P var. Max = 2426200 + 290d*E (JD2426000 - 30560)
V1577 Sgr    [02449]; since JD2430560 - see Table.
V1580 Sgr    P var (310d <= P <= 365d).
V1589 Sgr    [Ca/H] = -0.91.
V1602 Sgr    d = 0.03P.
V1610 Sgr    P < 0.5d.
V1639 Sgr    The shape of the light curve varies.
V1640 Sgr    (k -b)2 = 0.24. P var?
V1642 Sgr    250d <= P <= 350d.
V1643 Sgr    Min II 12.1. According to [05771], RR?, P = 0.34d.
V1644 Sgr    The shape of the light curve varies.
V1647 Sgr    VB A (B 9.13m, 8", 104deg). Min II 7.43, DII = 0.059P,
V1647 Sgr    Min II - Min I = 0.262P (JD2441830);
V1647 Sgr    Min II = 2441830.55561 + 3.28282227d*E.
V1647 Sgr    The apsidal motion period is 592.5 +- 6.5 years.
V1648 Sgr    Close VB. Flat Min.
V1652 Sgr    Close VB. Flat Min.
V1653 Sgr    Close VB. Flat Min.
V1656 Sgr    Close VB. Flat Min.
V1658 Sgr    P var.Max = 2426560 + 105d*E (JD2417000 - 28000)
V1658 Sgr    [00842]; since JD2428000 - see Table.
V1660 Sgr    Close VB. Flat Min.
V1661 Sgr    Close VB. Flat Min. P var. Max = 2426850 + 275d*E
V1661 Sgr    (JD2424000 - 26850); since JD2436700 - see Table.
V1667 Sgr    P var. Max = 2426560 + 158d*E (JD2417000 - 36000)
V1667 Sgr    [00842]; since JD2436000 - see Table.
V1668 Sgr    Close VB. Flat Min.
V1670 Sgr    A var. P var. The shape of the light curve varies
V1670 Sgr    (probably with a period of about 11 years).
V1675 Sgr    A possible companion of 16m.
V1679 Sgr    Close VB. Flat Min.
V1681 Sgr    A possible companion of 16m.
V1690 Sgr    A possible companion of 16m.
V1691 Sgr    Close VB. Flat Min.
V1691 Sgr    P var. Max = 2426520 + 235d*E (JD2417000 - 28000)
V1691 Sgr    [00842]; since JD2436000 - see Table.
V1697 Sgr    A possible companion of 16m.
V1698 Sgr    A possible companion of 16m.
V1699 Sgr    P var. Max = 2425410 + 203.6d*E (JD2417000 - 27600)
V1699 Sgr    [00842]; since JD2436000 - see Table.
V1703 Sgr    A possible companion of 16m.
V1705 Sgr    P var. Max = 2425860 + 142d*E (JD2417000 - 27000)
V1705 Sgr    [00842]; since JD2435800 - see Table.
V1711 Sgr    [A/H] = -1.1. P var. Max = 2435365.19 + 30.46d*E
V1711 Sgr    (JD2432700 - 35400) [02570]; since JD2442200 - see Table.
V1714 Sgr    In the region of the open cluster Ruprecht 134.
V1721 Sgr    d = 0.03P:.
V1723 Sgr    Min II 13.8.
V1730 Sgr    Min II 14.8:; d = 0.03P:.
V1741 Sgr    In the nebula and the cluster NGC 6530 (M8). Var1.
V1743 Sgr    In the nebula and the cluster NGC 6530 (M8). Var2.
V1747 Sgr    In the nebula and the cluster NGC 6530 (M8). Var3.
V1748 Sgr    In the nebula and the cluster NGC 6530 (M8). Var4.
V1749 Sgr    In the nebula and the cluster NGC 6530 (M8). Var6.
V1750 Sgr    In the nebula and the cluster NGC 6530 (M8). Var8.
V1751 Sgr    In the nebula and the cluster NGC 6530 (M8). Var7.
V1752 Sgr    In the nebula and the cluster NGC 6530 (M8). Var13.
V1753 Sgr    In the nebula and the cluster NGC 6530 (M8). Var14.
V1755 Sgr    In the nebula and the cluster NGC 6530 (M8). Var15.
V1758 Sgr    In the nebula and the cluster NGC 6530 (M8). Var16.
V1761 Sgr    In the nebula and the cluster NGC 6530 (M8). Var19.
V1762 Sgr    In the nebula and the cluster NGC 6530 (M8). Var20.
V1764 Sgr    In the nebula and the cluster NGC 6530 (M8). Var23.
V1765 Sgr    In the nebula and the cluster NGC 6530 (M8). Var24.
V1768 Sgr    In the nebula and the cluster NGC 6530 (M8). Var26.
V1769 Sgr    In the nebula and the cluster NGC 6530 (M8). Var27.
V1771 Sgr    In the nebula and the cluster NGC 6530 (M8). Var29.
V1772 Sgr    In the nebula and the cluster NGC 6530 (M8). Var28.
V1773 Sgr    In the nebula and the cluster NGC 6530 (M8). Var31.
V1774 Sgr    In the nebula and the cluster NGC 6530 (M8). Var30.
V1775 Sgr    In the nebula and the cluster NGC 6530 (M8). Var33.
V1776 Sgr    In the nebula and the cluster NGC 6530 (M8). Var36.
V1777 Sgr    In the nebula and the cluster NGC 6530 (M8). Var37.
V1778 Sgr    In the nebula and the cluster NGC 6530 (M8). Var34.
V1779 Sgr    In the nebula and the cluster NGC 6530 (M8). Var40.
V1780 Sgr    In the nebula and the cluster NGC 6530 (M8). Var39.
V1781 Sgr    In the nebula and the cluster NGC 6530 (M8). Var41.
V1782 Sgr    In the nebula and the cluster NGC 6530 (M8). Var44.
V1784 Sgr    In the nebula and the cluster NGC 6530 (M8). Var45.
V1785 Sgr    In the nebula and the cluster NGC 6530 (M8). Var46.
V1786 Sgr    In the nebula and the cluster NGC 6530 (M8). Var48.
V1787 Sgr    In the nebula and the cluster NGC 6530 (M8). Var47.
V1788 Sgr    In the nebula and the cluster NGC 6530 (M8). Var50.
V1789 Sgr    In the nebula and the cluster NGC 6530 (M8). Var51.
V1790 Sgr    In the nebula and the cluster NGC 6530 (M8). Var49.
V1790 Sgr    Western component of a close pair.
V1791 Sgr    In the nebula and the cluster NGC 6530 (M8). Var53.
V1792 Sgr    In the nebula and the cluster NGC 6530 (M8). Var55.
V1793 Sgr    In the nebula and the cluster NGC 6530 (M8). Var54.
V1794 Sgr    In the nebula and the cluster NGC 6530 (M8). Var56.
V1795 Sgr    In the nebula and the cluster NGC 6530 (M8). Var58.
V1797 Sgr    In the nebula and the cluster NGC 6530 (M8). Var59.
V1798 Sgr    In the nebula and the cluster NGC 6530 (M8). Var60.
V1800 Sgr    In the nebula and the cluster NGC 6530 (M8). Var61.
V1801 Sgr    In the nebula and the cluster NGC 6530 (M8). Var62.
V1802 Sgr    In the nebula and the cluster NGC 6530 (M8). Var63.
V1803 Sgr    In the nebula and the cluster NGC 6530 (M8). Var64.
V1803 Sgr    SP component of a close pair.
V1805 Sgr    In the nebula and the cluster NGC 6530 (M8). Var66.
V1807 Sgr    In the nebula and the cluster NGC 6530 (M8). Var67.
V1808 Sgr    In the nebula and the cluster NGC 6530 (M8). Var68.
V1828 Sgr    P var. Max = 2424402 + 12.985d*E (JD2423800 - 36000)
V1828 Sgr    [02515]; since JD2436000 - see Table.
V1831 Sgr    P var. Max = 2428849.4 + 26.58d*E (JD2427500 - 31270)
V1831 Sgr    [02447]; since JD2435630 - see Table.
V1843 Sgr    P = 163.7d? [05869].
V1845 Sgr    Flat Min. Close companion?
V1864 Sgr    Epoch of light maximum is given.
V1869 Sgr    P var. Max = 2434178 + 346d*E (JD2427590 - 34220)
V1869 Sgr    [02447]; since JD2435630 - see Table.
V1882 Sgr    The shape of the light curve varies.
V1891 Sgr    A companion of 16m.
V1894 Sgr    V4 (NGC 6637). Possible member of the globular cluster
V1894 Sgr    NGC 6637 (M 69).
V1895 Sgr    P var. Max = 2421065 + 156.0d*E (JD2418850 - 21100);
V1895 Sgr    since JD2427600 - see Table.
V1900 Sgr    A companion of 15m.
V1904 Sgr    A companion of 15m.
V1911 Sgr    P var. Max = 2428832.4 + 10.0581d*E (JD2427600 - 34220)
V1911 Sgr    [02447]; since JD2435630 - see Table. The shape of the
V1911 Sgr    light curve varies?
V1925 Sgr    P var?
V1942 Sgr    In the region of the open cluster Ruprecht 147.
V1945 Sgr    In the region of the open cluster and the diffuse nebula
V1945 Sgr    NGC 6514 (M20).
V1946 Sgr    In the region of the open cluster and the diffuse nebula
V1946 Sgr    NGC 6514 (M20).
V1947 Sgr    In the region of the open cluster and the diffuse nebula
V1947 Sgr    NGC 6514 (M20). All the published charts
V1947 Sgr    for this variable are wrong. According to [09861] the
V1947 Sgr    star actually lies 1.1 mm south and 0.8 mm east of
V1947 Sgr    "D2" in fugure 3 published in [02428].
V1948 Sgr    In the region of the open cluster and the diffuse nebula
V1948 Sgr    NGC 6514 (M20).
V1949 Sgr    In the region of the open cluster and the diffuse nebula
V1949 Sgr    NGC 6514 (M20).
V1950 Sgr    In the region of the open cluster and the diffuse nebula
V1950 Sgr    NGC 6514 (M20).
V1951 Sgr    In the region of the open cluster and the diffuse nebula
V1951 Sgr    NGC 6514 (M20).
V1954 Sgr    VB(ro = 2"). P var.
V1954 Sgr    There is a nonlinear term in the elements:
V1954 Sgr    -4.1313d*10**(-8)*E**2.
V1958 Sgr    Min II 14.0.
V1962 Sgr    In the region of the open cluster and the
V1962 Sgr    diffuse nebula NGC 6618 (M 17).
V1963 Sgr    In the region of the open cluster and the diffuse nebula
V1963 Sgr    NGC 6618 (M 17).
V1966 Sgr    In the region of the open cluster and the diffuse nebula
V1966 Sgr    NGC 6618 (M 17).
V1969 Sgr    There are three close faint companions (15.8m-16.3m).
V1970 Sgr    In the region of the open cluster and the diffuse nebula
V1970 Sgr    NGC 6618 (M 17).
V1971 Sgr    In the region of the open cluster and the diffuse nebula
V1971 Sgr    NGC 6618 (M 17).
V1973 Sgr    In the region of the open cluster and the diffuse nebula
V1973 Sgr    NGC 6618 (M 17).
V1975 Sgr    In the region of the open cluster and the diffuse nebula
V1975 Sgr    NGC 6618 (M 17). The presence of a blue companion is
V1975 Sgr    possible.
V1976 Sgr    In the region of the open cluster and the diffuse nebula
V1976 Sgr    NGC 6618 (M 17).
V1977 Sgr    In the region of the open cluster and the diffuse nebula
V1977 Sgr    NGC 6618 (M 17).
V1980 Sgr    Min II 11.7; DII = 0.11P; Min II - Min I = 0.52P.
V1996 Sgr    VB.
V2003 Sgr    S 5.5/5. In the region of the open cluster M 25 (IC 4725).
V2007 Sgr    V 26 (NGC 6656 = M 22).
V2008 Sgr    P = 120 - 135d.
V2028 Sgr    In the region of the globular cluster NGC 6681 (M 70).
V2037 Sgr    A close companion is possible.
V2054 Sgr    P > 450d?
V2062 Sgr    The chart in [4233] is wrong.
V2064 Sgr    VB. Combined brightness of the star and the close
V2064 Sgr    companion was estimated. It is not clear which star is
V2064 Sgr    variable.
V2065 Sgr    NP component of a close binary.
V2094 Sgr    P < 0.5d.
V2106 Sgr    VB. Combined brightness of the components was estimated.
V2148 Sgr    VB. Combined brightness of the components was estimated.
V2148 Sgr    The variable is the northern component.
V2276 Sgr    P < 30d.
V2282 Sgr    Star L. In the region of the open cluster and the diffuse
V2282 Sgr    nebula NGC 6514 (M20). Late spectrum.
V2283 Sgr    Min II 10.59:. Apsidal motion with P = 560 years [07107]:
V2283 Sgr    0.739P (1898) <= Min II - Min I <= 0.797P (1965).
V2283 Sgr    There are periodic terms in the
V2283 Sgr    elements given in the Table:
V2283 Sgr    +0.5414d*sin(0.006deg*(E + 45019)) - 0.0995d*sin(0.012deg*
V2283 Sgr    (E + 45019)) + 0.0217d*sin(0.018deg*(E + 45019)); Min II =
V2283 Sgr    2438946.7619 + 3.4714231d*E - 0.5414d*sin(0.006deg*
V2283 Sgr    (E + 45019)) - 0.0995d*sin(0.012deg*(E + 45019)) - 0.0217d*
V2283 Sgr    sin(0.018deg*(E + 45019)).
V2284 Sgr    P var.
V2313 Sgr    Min II 16.8.
V2315 Sgr    P = 0.193d?
V2323 Sgr    Blue [08424].
V2341 Sgr    The epoch of Min brightness is given.
V2342 Sgr    V 17 (NGC 6626 = M28).
V2342 Sgr    The member of this globular cluster. Min II 13.5.
V2343 Sgr    A close companion of 14.5m.
V2346 Sgr    Cycles 50 - 100d.
V2349 Sgr    Min II 9.2.
V2351 Sgr    Min II 10.31.
V2352 Sgr    P var. There is a nonlinear term in the elements:
V2352 Sgr    0.0525d*E**2.
V2355 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2358 Sgr    In the region of the globular cluster NGC 6642.
V2359 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2360 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2361 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2362 Sgr    A close companion of 15m.
V2366 Sgr    P var. There is a nonlinear term in the elements:
V2366 Sgr    +0.6815d*10**(-9)*E**2.
V2367 Sgr    V28 (NGC 6656 = M22). Not a member of this globular cluster.
V2367 Sgr    P = 323d?
V2378 Sgr    Two close companions of 15.3m and 15.8m.
V2389 Sgr    P var?
V2391 Sgr    P = 189d?
V2413 Sgr    P var. The elements are valid in the interval
V2413 Sgr    JD2425440 - 30905.
V2416 Sgr    P.K. 7 +1G 2.
V2425 Sgr    E?
V2442 Sgr    P = 0.5d?
V2449 Sgr    Min II 17.4.
V2468 Sgr    Blue [08424].
V2471 Sgr    VB B (A 14.6m; B 8", 225deg).
V2493 Sgr    Blue [08424].
V2506 Sgr    P.K. 3 -4deg 6.
V2507 Sgr    Min II 14.6.
V2508 Sgr    Min II 14.1:.
V2509 Sgr    Min II 7.50.
V2510 Sgr    The epoch of Min brigtness is given. The elements given
V2510 Sgr    in the Table are valid since JD2427440.
V2520 Sgr    VB.
V2526 Sgr    The epoch of Min brightness is given.
V2526 Sgr    P var. Min = 2428699.5 + 31.3224d*E (JD2424100 - 31400)
V2526 Sgr    [05590]. Since JD2431400 - see Table.
V2529 Sgr    Min II 14.5. Twice shorter period is given in [05590].
V2540 Sgr    P var.
V2544 Sgr    VB?
V2552 Sgr    VB A (B 15.7m).
V2553 Sgr    There are two close companions.
V2562 Sgr    Northern component of a close pair. The companion is of
V2562 Sgr    16m.
V2563 Sgr    P var.
V2564 Sgr    P var?
V2565 Sgr    VB B (A 12.5m; B 90deg).
V2566 Sgr    P var. [Ca/H] = -0.52.
V2567 Sgr    [Ca/H] = -0.57.
V2568 Sgr    P var?
V2576 Sgr    P var. Max = 2426200 + 149d*E (JD2423500 - 27000);
V2576 Sgr    since JD2433000 - see Table.
V2577 Sgr    P var?
V2578 Sgr    VB. In the region of the globular cluster NGC 6642.
V2579 Sgr    P var. Max = 2429926.251 + 0.5911903d*E (JD2427590 -
V2579 Sgr    34200) [05590]; since JD2435600 - see Table.
V2584 Sgr    P var. Max = 2426564.347 + 0.534829d*E (JD2423940 -
V2584 Sgr    33860); since JD2437820 - see Table.
V2592 Sgr    In the region of the globular cluster NGC 6656 (M22).
V2593 Sgr    P var. Max = 2428780.349 + 0.5123825d*E
V2593 Sgr    (JD2427680 - 34200) [05590]; since JD2435600 - see Table.
V2594 Sgr    P var.
V2598 Sgr    A companion 15.8m. Spectrum description [06495].
V2601 Sgr    P.K. 12 -7deg 1.  The epoch of Min brightness is given.
V2616 Sgr    Min II 13.0.
V2617 Sgr    Min II 9.63.
V2620 Sgr    P = 185.6d?
V2625 Sgr    P = 0.75837d?
V2628 Sgr    P = 171d:?/205d:?/256d:?.
V2645 Sgr    P var?
V2649 Sgr    P = 143d:?
V2672 Sgr    P = 196.8d? /204.5d, /255.3d? /315.0d?
V2682 Sgr    P = 228.5d?
V2687 Sgr    P = 174d:?
V2703 Sgr    P = 270d:?
V2719 Sgr    SR?
V2731 Sgr    P = 147d:?
V2732 Sgr    P = 188.6d?
V2733 Sgr    P = 244d:?
V2736 Sgr    [Ca/H] = -1.45.
V2738 Sgr    [Ca/H] = -0.67.
V2740 Sgr    P = 269.0d?
V2745 Sgr    [Ca/H] = -1.15.
V2756 Sgr    P.K. 2 -5deg 1. The epoch of Min brightness is given.
V2763 Sgr    P = 216d:?
V2777 Sgr    [Ca/H] = -0.83.
V2783 Sgr    P = 265.0d?
V2789 Sgr    P = 255.5d?
V2798 Sgr    P = 244.5d?
V2816 Sgr    P = 250d:?
V2828 Sgr    P = 0.39669d?
V2830 Sgr    Cepheid?
V2833 Sgr    P = 224.0d?
V2834 Sgr    P = 275d:?
V2846 Sgr    P = 0.39659d?
V2868 Sgr    P = 235.5d?
V2876 Sgr    Min II 15.7:.
V2877 Sgr    P = 254.5d?
V2893 Sgr    P = 250d:?
V2900 Sgr    P = 0.49835d?
V2905 Sgr    Spectrum description [04452, 06495].
V2918 Sgr    P = 197d:?
V2937 Sgr    [Ca/H] = -0.75.
V2947 Sgr    RV Tau? Cepheid?
V2959 Sgr    P = 0.37233d?
V2962 Sgr    P = 209.5d?
V2967 Sgr    P = 0.68750d?
V2996 Sgr    RV Tau? Cepheid?
V3004 Sgr    [Ca/H] = -0.76.
V3005 Sgr    RV Tau? Cepheid?
V3016 Sgr    P var?
V3032 Sgr    P = 153d:?
V3033 Sgr    The coordinates given in [05869] are erroneous.
V3034 Sgr    P = 154d:?
V3038 Sgr    P = 252d:?
V3052 Sgr    RV Tau? Cepheid?
V3062 Sgr    EW? P = 0.59610d?
V3065 Sgr    P = 179.8d?/215.5d?
V3071 Sgr    P = 291d:?
V3072 Sgr    P = 194d:?
V3088 Sgr    P = 215d:?
V3105 Sgr    [Ca/H] = -0.82.
V3106 Sgr    P = 261d:?
V3111 Sgr    P = 182.8d?
V3127 Sgr    UG? Not red.
V3128 Sgr    Nova? Only one Max was observed.
V3170 Sgr    [Ca/H] = -0.82.
V3175 Sgr    P = 179.8d?
V3176 Sgr    P = 197d:?
V3179 Sgr    P = 297d:?
V3186 Sgr    [Ca/H] = -1.28.
V3196 Sgr    RV Tau? Cepheid?
V3207 Sgr    P = 237d:?
V3239 Sgr    P = 226d:?
V3249 Sgr    UG?
V3285 Sgr    P = 173.8d /196.2d?
V3294 Sgr    P = 121d:? /177d:?
V3295 Sgr    P = 197d:?
V3335 Sgr    RV Tau? Cepheid?
V3353 Sgr    P var?
V3356 Sgr    P = 239.5d?
V3365 Sgr    P = 197d:? /252d:?
V3388 Sgr    P = 125d:? /160d:?
V3395 Sgr    P = 159d:?
V3412 Sgr    Cepheid?
V3433 Sgr    P = 287.0d?
V3443 Sgr    P = 177.6d?
V3444 Sgr    P = 160d:?
V3459 Sgr    P var. The shape of the light curve varies.
V3467 Sgr    RV Tau? Cepheid?
V3473 Sgr    SR?
V3500 Sgr    RV Tau? Cepheid?
V3501 Sgr    Min II 15.7:.
V3508 Sgr    The member of the open cluster M25 (IC 4725).
V3511 Sgr    RV Tau? Cepheid?
V3536 Sgr    P = 239.5d?
V3537 Sgr    P = 318.0d?
V3551 Sgr    P = 165.2d? /201.0d?
V3560 Sgr    P = 181d:?
V3564 Sgr    Cepheid?
V3566 Sgr    P = 249.0d?
V3583 Sgr    P = 228.0d?
V3588 Sgr    [Ca/H] = -0.69.
V3625 Sgr    P = 294d:?
V3634 Sgr    P = 145d:?
V3645 Sgr    In the region of the open cluster M25 (IC 4725).
V3709 Sgr    P = 240.0d?
V3718 Sgr    P var. There is a nonlinear term
V3718 Sgr    in the elements: +0.865d*10**(-10)*E**2.
V3748 Sgr    P = 0.305327d?
V3765 Sgr    [Ca/H] = -0.78.
V3783 Sgr    In the region of the globular cluster NGC 6681 (M70).
V3784 Sgr    P = 176.4d?
V3788 Sgr    In the region of the globular cluster NGC 6723. Red.
V3791 Sgr    In the region of the open cluster and the diffuse nebula
V3791 Sgr    NGC 6514 (M20).
V3792 Sgr    VB A (B 8.92m, 13.3", 90deg). Min II 6.81.
V3792 Sgr    The range of the combined light variation is given in the
V3792 Sgr    Table. The shape of the light curve varies.
V3804 Sgr    Spectrum description [06495, 07099].
V3811 Sgr    P2 = 4d? Spectrum description [07099, 09845].
V3817 Sgr    VB A (B 16m).
V3819 Sgr    P var. There is a nonlinear term in the elements:
V3819 Sgr    +10**(-10)*E**2.
V3829 Sgr    A close companion.
V3832 Sgr    A close companion.
V3834 Sgr    Cepheid or eclipsing?
V3837 Sgr    P = 0.565d? [06383].
V3838 Sgr    VB A (B 15.8m).
V3841 Sgr    P var. Max = 2431970 + 358d*E (JD2423900 - 33000);
V3841 Sgr    since JD2433000 - see Table.
V3842 Sgr    A close companion with M2? Spectral class possibly exists.
V3843 Sgr    In the region of the globular cluster NGC 6642.
V3853 Sgr    V22 (NGC 6656 = M22). The member of this globular cluster.
V3855 Sgr    V31 (NGC 6656 = M22). Possible member of the cluster.
V3857 Sgr    According to [06278] the spectral class is M8.
V3867 Sgr    Under the chart S 4903 is printed erroneously instead of
V3867 Sgr    CSV 4309.
V3868 Sgr    P var. Max = 2426130 + 270d*E (JD2423900 - 33900);
V3868 Sgr    since JD2435700 - see Table.
V3874 Sgr    P var. Max = 2436035 + 115.3d*E (JD2426000 - 38000);
V3874 Sgr    since JD2438000 - see Table.
V3875 Sgr    P var. P = 358d (JD2424000 - 33800); since
V3875 Sgr    JD2435000 - see Table.
V3876 Sgr    P var. Max = 2430090 + 345d*E (JD2423900 - 32000);
V3876 Sgr    Max = 2436830 + 358d*E (JD2436000 - 41500) [06279];
V3876 Sgr    since JD2441400 - see Table.
V3879 Sgr    VB (Delta(m) = 2.6m, ro = 0.6").
V3880 Sgr    OH, SiO, H2O maser.
V3885 Sgr    Porb = 0.206d [04939].
V3885 Sgr    Besides the irregular variability high-frequency
V3885 Sgr    oscillations are sometimes observed with
V3885 Sgr    P1 = 29.0s, P2 = 30.15s and with amplitudes of 0.00028m.
V3885 Sgr    In the spectrum there are extremely broad absorption
V3885 Sgr    lines of HI and HeI. The Balmer lines have emission
V3885 Sgr    components. X-ray source.
V3886 Sgr    Type EB?
V3893 Sgr    Connected with a ring nebula.
V3894 Sgr    Min II 6.37. P var?
V3899 Sgr    In the region of the open cluster and the diffuse nebula
V3899 Sgr    NGC 6514 (M20).
V3900 Sgr    V7 (NGC 6522). Not a member of this globular cluster.
V3903 Sgr    The member of the open cluster Collinder 367.
V3903 Sgr    In the nebula Simeis 188.
V3907 Sgr    The epoch of Min brightness is given.
V3929 Sgr    P.K.5 -5deg 2.
V3961 Sgr    SB1 (Porb = 690d [09915]).
V4024 Sgr    SB.
V4032 Sgr    Not far from V1309 Sgr.
V4034 Sgr    Flat Min. Close companion?
V4046 Sgr    Flares (11.1m - 12.4m U).
V4048 Sgr    Min II 12.6; DII = 0.15P.
V4051 Sgr    In the region of the globular cluster NGC 6638.
V4051 Sgr    Not a member of the cluster.
V4052 Sgr    In the region of the globular cluster NGC 6638.
V4052 Sgr    Not a member of the cluster.
V4054 Sgr    In the region of the globular cluster NGC 6638.
V4054 Sgr    Not a member of the cluster.
V4055 Sgr    In the region of the globular cluster NGC 6638.
V4055 Sgr    Not a member of the cluster.
V4058 Sgr    d = 0.02P
V4060 Sgr    P var. Max = 2437846 + 283d*E (JD2436030 - 38970);
V4060 Sgr    since JD2438970 - see Table.
V4066 Sgr    d ~0.07P.
V4067 Sgr    V32 (NGC 6656 = M22).
V4067 Sgr    Not a member of the globular cluster.
V4068 Sgr    V17 (NGC 6656 = M22).
V4068 Sgr    Not a member of the globular cluster.
V4069 Sgr    V33 (NGC 6656 = M22).
V4069 Sgr    Not a member of the globular cluster.
V4390 Sgr    SB2 and speckle binary.
V4417 Sgr    The variability may be due to the fainter (B) component.
V4429 Sgr    A giant, according to HIPPARCOS data, despite the published
V4429 Sgr    luminosity class (V).
V4620 Sgr    In the region of the globular cluster NGC 6558.
V4955 Sgr    Close to the N of V4521 Sgr, the periods differ considerably.
V5099 Sgr    SU UMa-type cv.
V5112 Sgr    A symmetrical minimum lasted for several months, with variations also outside it.
V5129 Sgr    MinII 15.71.
V5157 Sgr    The type was confirmed spectroscopically in [222].
V5164 Sgr    MinII 13.31.
V5325 Sgr    The Mira V3978 Sgr is in 12" to the west.
V5400 Sgr    The coordinates are given for BMB 21. BMB 20 5" np. It is not clear which component varies.
V5431 Sgr    VB A (B 5" np). It is not clear which component varies.
V5521 Sgr    MinII 15.8.
V5527 Sgr    MinII 16.9.
V5528 Sgr    MinII 17.7.
V5533 Sgr    The light curve with P = 0.94741 d in [022] is not convincing, our period is based on ASAS-3 data.
V5535 Sgr    MinII 10.96.
V5555 Sgr    A protoplanetary object, rapid irregular brightness variations.
V5559 Sgr    A twice shorter period is not excluded.
V5565 Sgr    MinII - MinI = 0.41P.
V5566 Sgr    VB A (B 7.5mKs, 7", 327deg, 1999). The A component looks not round on DSS images, the spectral type M6: [127] probably refers to an unresolved companion and not to component B.
V5569 Sgr    Besides eclipses, complex variations of different nature.
V5627 Sgr    A decline from 15.1m to 16.9m was observed between JD 2449800 and 2451400. The tabulated light elements are for eclipses in quiescence (Max 16.88m).
V5631 Sgr    VB A (B 11.2m, 1".9, 98deg, 2002).
V5632 Sgr    OH maser.
V5633 Sgr    Multiperiodic.
V5634 Sgr    X-ray pulses with P = 5.539917s.
V5639 Sgr    VB A (B 11.6m, 8", 142deg, 2000; several fainter companions).
V5640 Sgr    Erroneously called V1592 Sgr in [80502].
V5641 Sgr    Multiperiodic, P2 = 0.203290d.
V5644 Sgr    The fundamental period is tabulated; for the first overtone, P = 0.34247d.
V5649 Sgr    Blended, combined magnitudes are tabulated. Type Mira is not excluded.
V5659 Sgr    Blazhko effect, P = 45.69d.
V5664 Sgr    Type EW with a twice longer period is possible.
eta   Sgr    VB A (B 8.0m, 3.5",105deg); mu alpha = -0.0107s,
eta   Sgr    mu delta = -0.166".
mu.   Sgr    VB A (B 10.48m, 16.9", 285deg; C 13.0m, 25.2", 119deg;
mu.   Sgr    D 9.69m, 48.5", 312deg; E 9.25m, 50.0", 115deg). SB2
mu.   Sgr    (e = 0.4). The variability type is EA/GS + ACYG.
mu.   Sgr    According to [09922] there are also quasiperiodical light
mu.   Sgr    variations with the amplitudes 0.08m - 0.15m and cycles
mu.   Sgr    from 16d to 40d.
ups   Sgr    Min II 4.59.
R     Sco    V7 (NGC 6093 = M80). Probable field star.
R     Sco    P var. Max = 2400518 + 220.2d*E (JD2400500 - 04000)
R     Sco    [00960]; Max = 2404493 + 225.86d*E (JD2404000 - 08600);
R     Sco    Max = 2409003 + 222.29d*E (JD2408600 - 33300); since
R     Sco    JD2433300 - see Table.
S     Sco    V6 (NGC 6093 = M80). Cluster non-member.
S     Sco    P var. Max = 2400986 + 177.00d*E (JD2400900 - 17500);
S     Sco    since JD2417500 - see Table.
T     Sco    4.0" N, 2.7" E from the center of the globular cluster
T     Sco    NGC 6093 = M80.
U     Sco    Previous outbursts:
U     Sco    2401646: (1863), 2417343 (1906), 2428342 (1936).
Y     Sco    Since 1972 varies its brightness in the range 12.3m-15.0m
Y     Sco    irregularly, maxima are unpredictable [08080].
Z     Sco    P var. Max = 2425546 + 357.17d*E (JD2412500 -
Z     Sco    25600); since JD2430000 - see Table.
RR    Sco    SiO maser. P var. Max = 2416944 + 284.31d*E
RR    Sco    (JD2411000 - 18000); Max = 2422828 + 278.09d*E
RR    Sco    (JD2422800 - 40000); since JD2440000 - see Table.
RU    Sco    P var. During JD2425000 - 40000 - see Table.
RV    Sco    VB A (B 13.0m, 5.9", 325deg).
RW    Sco    OH, H2O, SiO maser.
RY    Sco    P var, nonlinear term: +4.10d*10**(-6)*E**2. [A/H] = 0.2.
RY    Sco    VB A (B 10.70m, F8:, 13.8", 220.5deg, 1965;
RY    Sco    C 11.5m, 2.0", 102deg, 1964; D 11.43m, 24", 80deg).
RY    Sco    Combined brightness of AC is given.
RZ    Sco    P var. Max = 2413994 + 161.20d*E (JD2413600 - 22700);
RZ    Sco    Max = 2422858 + 155.79d*E (JD2422700 - 28000);
RZ    Sco    Max = 2428156  +  160.29d*E (JD2428000 - 35000); since
RZ    Sco    JD2437500 - see Table.
SV    Sco    P var. Max = 2418886 + 258.5d:*E (JD2411600 - 19000);
SV    Sco    Max = 2424233 + 252.43d*E (JD2420500 - 28600);
SV    Sco    Max = 2429055 + 255.9d:*E (JD2428600 - 35000);
SV    Sco    since JD2437000 - see Table.
SY    Sco    In the region of the open cluster NGC 6475 = M7.
TX    Sco    In the region of the open cluster NGC 6475 = M7.
TX    Sco    Probable cluster member.
XX    Sco    The elements Max = 2413786 + 152d*E
XX    Sco    [00031] do not represent the observations from [09447].
AC    Sco    According to [00266], CST:, 12.2m - 12.6m pg.
AH    Sco    OH, H2O, SiO maser.
AI    Sco    P2 = 966.6d.
AL    Sco    Min II 11.3.
AN    Sco    EA type is possible.
AP    Sco    The chart in [09447] is wrong.
AR    Sco    According to [07104], T Tau type spectrum.
AU    Sco    VB A (B = V725 Sco, 0.4', 0deg).
AV    Sco    The chart and data in [09447] correspond to another star.
BI    Sco    VB B (A = GW Sco; B 6", 150deg).
BM    Sco    In the region of the open cluster NGC 6405 = M6.
BN    Sco    In the region of the open cluster NGC 6475 = M7.
BN    Sco    Resembles R Cen.
BS    Sco    d <= 0.03P. According to [00021], SP F8.
BT    Sco    P var. There is periodic term in the elements given in the
BT    Sco    Table: +0.05d*sin(176deg + 0.0857deg*E). Blazhko effect?
BV    Sco    Doubtful identification in [09447].
CF    Sco    Min II 13.8.
CK    Sco    VB A (B 15m, 14").
CL    Sco    The brightness in optical and UV range is modulated
CL    Sco    according to the elements: Min (pg) = 2427020 + 624.7d*E.
CL    Sco    Outbursts 1892, 1899, 1907, 1926.
CP    Sco    N /= 4.
CQ    Sco    [A/H] = -1.4.
DX    Sco    VB A (B p).
EZ    Sco    VB A (B 15.6m nf).
FQ    Sco    VB A (B 16m vis).
FU    Sco    VB A (B np). Min II 12.7, Min II - MiN I = 0.493P.
FV    Sco    d = 0.015P. Depth of Min II 0.1m pg.
FY    Sco    VB A (B 15m, 15", 35deg).
GG    Sco    VB A (B 15m, 8", 45deg).
GM    Sco    The nothern one of the two stars noted on the chart for
GM    Sco    SVS 1677.
GW    Sco    VB A (B = BI Sco, 6", 150deg).
IU    Sco    VB A (B 16.4m nf).
IU    Sco    Max = 2413280 + 69.05d*E (1893 - 1906);
IU    Sco    during 1910 - 1928 - see Table.
KO    Sco    Rapid variations: A = 1.0m. Slow changes:
KO    Sco    A = 0.5m, P = 2000d +-.
KQ    Sco    [A/H] = +0.3. P var?
LO    Sco    P var? Before JD2419150 Max = 2411500 + 450d*E;
LO    Sco    since JD2423900 - see Table.
LO    Sco    The spectrum is later than M5.
LR    Sco    The spectrum resembles RCrB in Max light [08090].
LR    Sco    IR excess. RCB type minima were not observed.
OO    Sco    In the region of the open cluster TR 29.
OQ    Sco    The chart in [06286] is wrong.
QZ    Sco    P var. Before JD2420400 Max = 2412640 + 158d*E;
QZ    Sco    since JD2423900 - see Table.
V0347 Sco    P var. Before JD2418700 Max = 2411500 + 198d*E;
V0347 Sco    since JD2423900 - see Table.
V0350 Sco    VB A (B 15.0m, 3", 233 deg).
V0381 Sco    d = 0.046P.
V0382 Sco    In the region of the open cluster NGC 6475 = M7.
V0385 Sco    In the region of the open cluster CR 338.
V0387 Sco    Min II 12.2.
V0390 Sco    P var. Before JD2422500 Max = 2420330 + 466d*E;
V0390 Sco    since JD2423900 - see Table.
V0393 Sco    Min II 8.3.
V0400 Sco    Min II 15.0.
V0402 Sco    In the region of the open cluster NGC 6475 = M7.
V0403 Sco    d ~0.02P. The depth of Min II 0.05m.
V0407 Sco    In the region of the open cluster NGC 6475 = M7.
V0411 Sco    Min II 14.0.
V0412 Sco    Min II 14.8. In the region of the open cluster
V0412 Sco    NGC 6475 = M7.
V0420 Sco    In the region of the open cluster NGC 6475 = M7.
V0421 Sco    P var. Before JD2418000 Max = 2413830 + 293d*E;
V0421 Sco    since JD2423900 - see Table.
V0423 Sco    Min II 14.2. In the region of the open cluster
V0423 Sco    NGC 6475 = M7.
V0425 Sco    In the region of the open cluster NGC 6475 = M7.
V0426 Sco    In the region of the open cluster NGC 6475 = M7.
V0429 Sco    In the region of the open cluster NGC 6475 = M7.
V0430 Sco    In the region of the open cluster Tr 30.
V0432 Sco    In the region of the open cluster Tr 30.
V0437 Sco    d = 0.02P. Min II 13.9.
V0439 Sco    P var. Before JD2418200 Max = 2413350 + 166.5d*E;
V0439 Sco    since JD2419900 - see Table.
V0440 Sco    In the region of the open cluster Tr 30.
V0446 Sco    P var? before JD2435000 Max = 2434980.1 +
V0446 Sco    28.6195d. [A/H] = -1.0.
V0450 Sco    A = 0.9m pg.
V0453 Sco    VB A (B 13.51m, F7V, 13.5", 168deg). Min II 6.70.
V0453 Sco    The light curve shape var?
V0455 Sco    P.K.351deg  + 3deg1. Planetary nebula nature is doubtful.
V0455 Sco    Nova-like outbursts separated by several years.
V0457 Sco    Min II 11.3.
V0460 Sco    d = 0.02P.
V0464 Sco    d = 0.03P.
V0466 Sco    Min II 13.7.
V0467 Sco    P var. P = 2.41354d (1889 - 1903); since 1903 - see Table.
V0470 Sco    [A/H] = 0.1.
V0471 Sco    Min II 15.2, dII = 0.08P(!).
V0472 Sco    d = 0.02P.
V0474 Sco    Min II 10.6.
V0483 Sco    CI = +3.5m.
V0485 Sco    Short term variations are superimposed.
V0486 Sco    D >= 4d? P = 1d is possible. In the region of
V0486 Sco    the open cluster NGC 6383.
V0487 Sco    [Fe/H] = -1.67, Delta(S) = 9.0.
V0490 Sco    Min II 12.5.
V0491 Sco    Min II 13.2.
V0494 Sco    A var (1.27m - 1.66m B). P var? Delta(S) = 2.
V0494 Sco    VB A (B 12.72m y, 23").
V0495 Sco    Short term variation are superimposed.
V0495 Sco    (Delta(m)short = 0.5m +-).
V0496 Sco    In the region of the open cluster NGC 6414.
V0496 Sco    d = 0.03P.
V0497 Sco    Min II 13.6.
V0499 Sco    AII = 0.47m V. Min I - Min II = 0.504P.
V0502 Sco    In the region of the open cluster C 1712 - 407.
V0507 Sco    The epoch of Max from [00300] contradicts the elements.
V0540 Sco    VB A (B 15.2m sp).
V0547 Sco    VB B (A 14.2m sf).
V0549 Sco    [A/H] = -1.1.
V0555 Sco    [A/H] = -0.3.
V0562 Sco    Min II 12.1.
V0566 Sco    d = 0.01P:.
V0567 Sco    VB A (B 13.01m, 10"sp, CD 30"nf). P var.
V0568 Sco    d = 0.04P.
V0569 Sco    Min II 11.4.
V0570 Sco    P var? Unusually broad Max.
V0573 Sco    d = 0.06P. In the region of the open cluster Tr 24.
V0574 Sco    In the region of the open cluster Tr 24.
V0575 Sco    Min II 12.4.
V0579 Sco    In the region of the open cluster Tr 24.
V0581 Sco    Min II 11.9.
V0584 Sco    Min II 13.1.
V0585 Sco    d = 0.03P:.
V0586 Sco    d = 0.04P. In the region of the open cluster Tr 24.
V0588 Sco    d = 0.02P. In the region of the open cluster Tr 24.
V0589 Sco    d = 0.05P. In the region of the open cluster Tr 24.
V0590 Sco    In the region of the open cluster NGC 6231.
V0592 Sco    Min II 13.3.
V0593 Sco    d = 0.05P:.
V0594 Sco    d = 0.01P.
V0603 Sco    d = 0.04P.
V0606 Sco    d = 0.07P.
V0607 Sco    Min II 10.3.
V0609 Sco    Min II 13.7.
V0611 Sco    d = 0.04P. Min II 13.7.
V0612 Sco    d = 0.05P.
V0613 Sco    d = 0.04P.
V0616 Sco    Min II 12.4.
V0619 Sco    Min II 12.1.
V0620 Sco    d = 0.02P.
V0621 Sco    d = 0.04P.
V0622 Sco    Min II 14.2.
V0623 Sco    Long intervals in Max without changes, sometimes becomes
V0623 Sco    faint.
V0625 Sco    VB A (B 13.2m sf). Min II 13.5.
V0627 Sco    Min II 14.1.
V0628 Sco    Min II 12.4.
V0629 Sco    Apsidal motion.
V0631 Sco    Min II 13.2.
V0632 Sco    d = 0.06P.
V0633 Sco    Min II 12.2.
V0634 Sco    Min II 12.2.
V0636 Sco    SB1 (Porb = 1318d).
V0638 Sco    d = 0.07P.
V0640 Sco    Min II 13.5.
V0656 Sco    The chart in [06286] is wrong.
V0660 Sco    VB A (B 16.0m s).
V0672 Sco    P = 180d is possible.
V0674 Sco    VB A (B 15.0m s).
V0677 Sco    The chart in [06286] is wrong.
V0679 Sco    P = 364d is possible.
V0690 Sco    VB A (B 14.40m y, 6", 0deg). The range of the combined
V0690 Sco    light is given. Delta(S) = 4.
V0698 Sco    D <= 0.20d, d = 0.043d.
V0700 Sco    Min II 10.3.
V0701 Sco    Min II 9.05. P var. Min I = 2439329.6657 + 0.76187133d*E
V0701 Sco    (JD2428000 - 39400) [07177]; since JD2439400 - see Table.
V0701 Sco    Probable member of the open cluster NGC 6383.
V0702 Sco    Probable member of the open cluster NGC 6383.
V0703 Sco    P0 = 0.1499615d [03521]; P1 - see Table
V0703 Sco    (P var?). Also noted P = 0.04162025d [03521].
V0703 Sco    A var (0.23m - 0.46m). Beat phenomenon:
V0703 Sco    Max = 2436760.249 + 0.497306d*E [03521]. Delta(S) = 1.
V0703 Sco    In the region of the open cluster NGC 6405 = M6.
V0705 Sco    Min II 14.1:.
V0706 Sco    Moments of Max from [00046] contradict the tabulated
V0706 Sco    elements. According to [04678], A <= 0.05m V
V0706 Sco    during 6 nights.
V0708 Sco    In the region of the open cluster NGC 6475 = M7.
V0709 Sco    IN the region of the open cluster NGC 6475 = M7.
V0709 Sco    [A/H] = -0.6.
V0710 Sco    Min II 14.2.
V0711 Sco    In the region of the open cluster NGC 6475 = M7.
V0712 Sco    Min II 14.0.
V0714 Sco    d = 0.05P:. P may be twice longer.
V0717 Sco    [A/H] = 0.9.
V0718 Sco    D ~4d. Another Min 2429847 - 849 [00270].
V0720 Sco    In the region of the open cluster NGC 6475 = M7.
V0723 Sco    In the region of the open cluster NGC 6475 = M7. At the
V0723 Sco    edge of a dark cloud.
V0725 Sco    VB B (A = AU Sco, B 0.4', 0deg).
V0729 Sco    Possibly a Nova.
V0732 Sco    P may be twice longer.
V0733 Sco    Possibly a Nova.
V0734 Sco    Possibly a Nova.
V0735 Sco    The light curve shape var.
V0738 Sco    d = 0.04P:; Min II 13.4:. In the region of the open
V0738 Sco    cluster NGC 6475 = M7.
V0740 Sco    In the region of the open cluster NGC 6475 = M7.
V0741 Sco    There is a red variable close to the coordinates in the
V0741 Sco    discovery announcement [02448], but a different star is
V0741 Sco    marked in the chart in [02448].
V0749 Sco    P = 410d is possible.
V0751 Sco    Erroneously named HV 9160 and CSV 3584 in [02448].
V0756 Sco    Min II 10.7.
V0760 Sco    dI = 0.02P; Min II 7.4; DII = 0.2P:, dII = 0.03P.
V0761 Sco    IN type is not excluded.
V0764 Sco    Min II 9.0.
V0805 Sco    Possibly P is twice shorter.
V0818 Sco    Sco X-1. SB.
V0818 Sco    Var X-ray and multi-component radio source.
V0818 Sco    Lx/Lbol = 300 - 1000. The epoch of Min is
V0818 Sco    given for the periodic component of the light variation
V0818 Sco    (A ~0.25m). Flickering and flares up to 1m with
V0818 Sco    time scale from dozens of seconds to minutes. The
V0818 Sco    mean brightness level decreased in the middle of
V0818 Sco    1960-es by 0.3m-0.4m. The spectrum with blue continuum
V0818 Sco    and H, HeI, HeII, CIII, NIII emissions.
V0819 Sco    Min II 13.2.
V0821 Sco    Min II 14.5.
V0822 Sco    VB? Combined brightness.
V0827 Sco    Min II 14.1.
V0833 Sco    Min II 11.2.
V0837 Sco    d ~0.03P:; Min II 14.3.
V0838 Sco    Min II 13.4.
V0842 Sco    Min II 12.3.
V0843 Sco    Min II 10.5.
V0848 Sco    Min II 13.1. RRC type with twice shorter period is
V0848 Sco    possible.
V0849 Sco    Min II 14.1.
V0853 Sco    d = 0.05P; Min II 14.1.
V0856 Sco    VB C (A = BS 6000, 6.65m, AO-3III; B 12.55m, 16",
V0856 Sco    298deg; C 44", 185deg; D 11.7m, CD 1.3", 105deg, 1945).
V0857 Sco    Erroneously labelled "10" (instead of "11") in the chart.
V0858 Sco    Erroneously labelled "11" (instead of "10") in the chart.
V0861 Sco    SB1. Min II 6.28. Depths of minima var. In the region of
V0861 Sco    the open cluster NGC 6231, Cr 316, Tr 24.
V0862 Sco    Usually 6.67m - 6.76m. A flare of 40m duration on July 3,
V0862 Sco    1965. In the region of the open cluster NGC 6405 = M6.
V0866 Sco    VB (Delta(m) ~0.5m, ~1", 200deg). m (6370 A) =
V0866 Sco    11.14m - 12.37m. IR excess.
V0870 Sco    B-V =  +3.38m - +3.52m. In the region of the open cluster
V0870 Sco    NGC 6231.
V0877 Sco    Min II 13.1.
V0883 Sco    VB A (B 12.60m, 9", 130deg). P var?
V0883 Sco    Min = 2438228.315 + 1.294745d*E (JD2438200 - 40500)
V0883 Sco    [06871]; since JD2440500 - see Table. Deep Min II.
V0884 Sco    4U 1700-37. LX/Lbol = 0.00007.
V0884 Sco    Eclipsing X-ray source. Eclipse duration is variable
V0884 Sco    in the ranges 0.61d <= dx <= 1.10d. The epoch of the
V0884 Sco    middle of the X-ray eclipse coinciding with Min II is
V0884 Sco    given. X-ray flux var in the scale from seconds till
V0884 Sco    hours. Sometimes a periodic modulation with P ~97
V0884 Sco    Min is present, its amplitude in the optical band reaches
V0884 Sco    Delta(V) ~0.01m. Min II 6.57; Min I - Min II = 0.63P,
V0884 Sco    dI=0.2P. Surrounded by the ring nebula Sh 2. in the region
V0884 Sco    of the open cluster NGC 6281. Field star.
V0885 Sco    Noticeable Min II.
V0889 Sco    The northern component of a triple.
V0890 Sco    VB A (B 11.5m, 0.5' n).
V0894 Sco    A = 0.6m pg.
V0896 Sco    Co-ordinates or the chart may be erroneous.
V0900 Sco    In the region of the open cluster NGC 6231.
V0900 Sco    The light curve is a sinusoidal wave. Possibly
V0900 Sco    P = 6.20d; 6.85d.
V0903 Sco    N96 [02448]. Erroneously identified with V479 Sco.
V0906 Sco    In the region of the open cluster NGC 6475 = M7. Probable
V0906 Sco    cluster member. VB (delta(mV) = 0.8m, 0.1", 111deg, 1957).
V0906 Sco    The range of the combined light variation is given.
V0906 Sco    Min II 6.21.
V0907 Sco    In the region of the open cluster NGC 6475 = M7.
V0907 Sco    Min II 9.2.
V0911 Sco    Alternative P = 4.2d.
V0913 Sco    Alternative P = 0.976d. IR excess.
V0914 Sco    VB (delta(mV) = 2m, 3", 200deg). Sine wave with P = 2.69d,
V0914 Sco    Delta(B) = 0.15m (B = 12.91m) [09753].
V0915 Sco    VB A (B 10.43m, WN6, 14", 330deg; C 11.40m, 20", 202deg;
V0915 Sco    D 13.96m, 22", 80deg, 1973). The brightness decreased from
V0915 Sco    6.32m to 6.50m during JD2443680 - 44115.
V0917 Sco    VB A (B 17m: sp). The outburst: rise 1930-1936,
V0917 Sco    Max 1936-1938, decline 1938-1952.
V0919 Sco    In the region of the open cluster NGC 6231.
V0920 Sco    In the region of the open cluster NGC 6231. Multiple
V0920 Sco    periodicity: P1 - see Table, semiamplitude A1 = 0.0051m;
V0920 Sco    P2 = 0.10765d. A2 = 0.0046m; P3 = 0.10388d, A3 = 0.00485m;
V0920 Sco    P4 = 0.12137d, A4 = 0.0036m; P5 = 0.6929d?, A5 = 0.0028m.
V0921 Sco    The star illuminates a nebula.
V0922 Sco    Multiple periodicity, superposition of frequencies with
V0922 Sco    amplitudes 0.0010m - 0.0352m.
V0923 Sco    D = 0.32d:. The elements need confirmation. In the region
V0923 Sco    of the open cluster NGC 6281.
V0924 Sco    B-V var: +1.90, +2.50,
V0924 Sco    Light fluctuations by 0.1m - 0.2m (u, b) in several
V0924 Sco    minutes.
V0925 Sco    VB A (B ~10", faint, blue). Probable member of the open
V0925 Sco    cluster TR 27. In Vr possible values of P: 105.3d, 73.0d,
V0925 Sco    188.7d, 312.5d [09950].
V0926 Sco    3U 1735-44 = Sco XR-3. Bursts superimpose small light
V0926 Sco    variations with P = 0.18d which is apparently the
V0926 Sco    orbital period [04394].
V0927 Sco    The epoch of Min in U light is given. IR excess.
V1195 Sco    MinII 9.01 at phase 0.4.
V1196 Sco    Symbiotic spectrum.
V1212 Sco    The magnitude in [189] refers to a different star but the period is correct [040].
V1216 Sco    MinII 10.35.
V1225 Sco    MinII 10.25.
V1229 Sco    MinII 8.96.
V1230 Sco    Erroneously called V719 Sco in [218].
V1270 Sco    MinII 9.70.
V1279 Sco    B - V: +1.23, +1.46.
V1286 Sco    Very red, J - K = 1.35 (2MASS).
V1292 Sco    MinII - MinI = 0.44P.
V1296 Sco    MinII - MinI = 0.56P.
V1299 Sco    MinII - MinI = 0.55P.
V1300 Sco    A twice shorter period is not excluded.
V1301 Sco    MinII - MinI = 0.53P.
V1302 Sco    A twice shorter period is not excluded.
V1303 Sco    MinII - MinI = 0.34P:.
V1305 Sco    VB (9.0m, 11.8m, 1.0", 153deg, 1927).
V1308 Sco    MinII - MinI = 0.48P.
V1317 Sco    One deep fading has been detected. After JD 2454100, a cycle of 58.4d (amplitude 0.7m) was observed.
V1319 Sco    P varies. Before JD 2452258, Max = 2452053.713 + 0.2541756d x E. The tabulated light elements are valid after JD 2452258.
V1327 Sco    VB (0.3", 5deg, 1995).
V1331 Sco    In the region of the globular cluster M4. Cluster non-member.
V1364 Sco    Multiperiodic.
V1414 Sco    OH maser.
V1452 Sco    Multiperiodic.
V1485 Sco    VB A (B 15.6m, 7", 244deg, 1999).
V1488 Sco    VB A (9.56mJ; B 9.74mJ, 6", 245deg, 1999).
V1504 Sco    The long period is about 735d.
V1506 Sco    VB A (B 14.04m, 10", 333deg, 2000; several other components. Second periodicity: P = 0.423350d or twice shorter.
V1512 Sco    P2 = 0.058920d. VB AB (10.6, 11.0, 0".5, 204deg, 1991).
V1517 Sco    Foreground star, globular cluster non-member.
V1520 Sco    Foreground star, globular cluster non-member.
alf   Sco    ADS 10074 A(B 5.1m, B4Ve, A = 2.9", Porb = 878 yr.).
alf   Sco    Connected with a nebula.
zet 1 Sco    In the region of the open cluster NGC 6231.
kap   Sco    SB. P2 = 0.205430d. P1 var. Beat phenomenon:
kap   Sco    Pi = 7.3316d.
lam   Sco    SB1. Porb = 5.6d? Apuls = 0.02m. Long period light changes:
lam   Sco    Max = 2440376.15 + 10.1605d*E [09761]. One eclipse was
lam   Sco    found (JD2440690, A ~0.04m) [06388].
mu. 1 Sco    Min II 3.12.
sig   Sco    VB AA (A 5.5m, 0.37", 96deg, 1981,
sig   Sco    orbital motion?; B 8.45m, B9.5V, 20.1", 273deg,
sig   Sco    1961); SB1, Porb = 33.06d. P0 var.
sig   Sco    Max Vr = 2420000.1465 + 0.24682815d*E (1918 - 1924)
sig   Sco    [09953]; Max = 2432306.918 + 0.246846d*E (JD2432000 - 37800)
sig   Sco    [09764]; since JD2437800 - see Table.
sig   Sco    A0 = 0.036m y. P1 = 0.2396674d, A1 = 0.013m y [09762].
sig   Sco    Pbeat = 8.256d = Porb/4 [09957].
sig   Sco    Connected with a nebula.
R     Scl    VB A (B 19.9m, 10", 234deg). CO emission.
S     Scl    P var. Max = 412774 + 367.9d*E (JD2405400 - 20500);
S     Scl    Max = 2423035 + 360.6d*E (JD2421250 - 27740);
S     Scl    Max = 2427738 + 370.4d*E (JD2427700 - 34000) [00960];
S     Scl    Since JD2434000 - see Table. H2O emission.
T     Scl    P var. Max = 2417400 + 202.26d*E (JD2411300 - 19000);
T     Scl    Max = 2420390 + 197.85d*E (JD2419000 - 23600);
T     Scl    since JD2423600 - see Table.
V     Scl    P var. Max = 2414006 + 294.8d*E (JD2411600 - 18200);
V     Scl    Max = 2422866 + 297.2d*E (JD2420400 - 35100);
V     Scl    since JD2435100 - see Table.
X     Scl    P var. Max = 2413796 + 258.7d*E (JD2413500 - 22800);
X     Scl    since JD2422800 - see Table.
Y     Scl    The cycles 100d: and 300d: are sometimes observed.
RT    Scl    Min II 10.47. [Fe/H] = -0.75. P var. There is
RT    Scl    a nonlinear term in the elements given in the Table:
RT    Scl    -9.04d*10**(-11)*E**2.
RU    Scl    (k - b)2 = 0.09. A var [03429]. P var. Max = 2425094.4175 +
RU    Scl    0.4933257d*E (JD2416750 - 25100) [00183]; Max =
RU    Scl    2427403.177 + 0.4933239d*E (JD2425100 - 30650)
RU    Scl    [01381]; since JD2430650 - see Table.
RW    Scl    P var?
SV    Scl    [Fe/H] = -1.82. P var? Max = 2439468.364 +
SV    Scl    0.3773636d*E (JD2427300 - 39500) [05233];
SV    Scl    since JD2439850 - see Table.
SY    Scl    H2O maser. P var? Max = 2426160 + 411d*E [00193]; since
SY    Scl    JD2440400 - see Table.
SZ    Scl    Min II 13.68.
UY    Scl    Near the galaxy NGC 55.
UZ    Scl    VB A (B 15.81m, 23", 135deg); (k - b)2 = 0.14. The
UZ    Scl    shape of the light curve varies.
VV    Scl    Min II 8.50. ACV? [08083].
VY    Scl    Porb = 0.1662d? [09932]. High and low states of the
VY    Scl    system are observed.
VZ    Scl    High and low states of the system are observed [09933].
WZ    Scl    There are two oscillations with the periods P1 and
WZ    Scl    P2: P1 = 0.06576d, P2 = 0.095944d, P1/P2 = 0.6854.
XX    Scl    There are two oscillations with the periods P1 and
XX    Scl    P2: P1 = 0.048898d, P2 = 0.051350d, P1/P2 = 0.95225.
AI    Scl    There are two oscillations with the periods P1 and
AI    Scl    P2: P1 = 0.044d, P2 = 0.0931d, P1/P2 = 0.47.
AL    Scl    Min II 6.20; Min II - Min I = 0.475P; DII = 0.08P.
AO    Scl    mu = 0.46", P = 187deg.
BC    Scl    May be eclipsing.
BI    Scl    Type E: is also possible.
CE    Scl    Min II 9.75.
CI    Scl    MinII - MinI = 0.39P. VB (A 9.50mHp; B 9.82mHp, 0.8", 240deg, 1991).
CM    Scl    MinII - MinI = 0.40P. VB (9.0m, 10.8m, 1.0", 111deg, 1991).
CP    Scl    Min II = 13.01. P varies. dP/dt = -0.23x10^(-5) d/yr.
CQ    Scl    Min II = 12.40. P varies. dP/dt = -0.23x10^(-5) d/yr.
CR    Scl    Min II = 9.68. P varies. dP/dt = 0.26x10^(-5) d/yr. VB AB (A 9.8m; B 12.7m, 4", 231deg, 1975).
CT    Scl    Min II = 12.08.
CX    Scl    Light elements for eclipses are tabulated. DSCTC pulsations: P = 0.183038d, Delta m = 0.11m.
R     Sct    [Fe/H] = -1. P var. Min I = 2377165 + 142.8d*E
R     Sct    (JD2377160 - 9820); Min I = 2384885 + 142.6d*E
R     Sct    (JD2384890 - 8170); Min I = 2394451 + 141.4d*E
R     Sct    (JD2394450 - 8500); Min I = 2398777 + 142.4d*E
R     Sct    (JD2398770 - 2404320); Min I = 2404627 + 137.4d*E
R     Sct    (JD2404600 - 6410); Min I = 2406561 + 142.7d*E
R     Sct    (JD2406560 - 9065); Min I = 2409742 + 143.6d*E
R     Sct    (JD2409730 - 12700); Min I = 2412755 + 141.5d*E
R     Sct    (JD2412750 - 16720); Min I = 2417161 + 139.5d*E
R     Sct    (JD2417150 - 20790); Min I = 2421083 + 143.4d*E
R     Sct    (JD2421050 - 25170) [09935]; Min I = 2429478 + 142.8d*E
R     Sct    (JD2429000 - 30650) [09938]; Min I = 2432078 + 140.05d*E
R     Sct    (JD2432000 - 42240) [07596]; Min I = 2442737 + 152.5d*E
R     Sct    (JD2442550 - 43050); Min I = 2443315 + 138.5d*E
R     Sct    (JD2443050 - 44150) [00001]; since JD2444150 - see Table.
R     Sct    Light curve drawings [09935, 09936, 9937].
R     Sct    Spectrum description [09939, 09954].
S     Sct    VB A (B 11.9M V, 14.5", 238deg; C 12.5m V, 44", 105deg).
U     Sct    Min II 10.31.
W     Sct    Min II 10.1.
X     Sct    [A/H] = -0.1. In the region of the open cluster NGC 6639.
Y     Sct    In the region of the open cluster NGC 6664.
Z     Sct    [A/H] = 0.3.
RS    Sct    Min II 10.08.
RU    Sct    [A/H] = -0.7. P var. There is a nonlinear term in the
RU    Sct    elements given in the Table: +3.15d*10**(-6)*E**2.
RX    Sct    Connected with the bright hydrogen nebula YM 13.
RY    Sct    Min II 9.56. P var? Min I = 2427979.340 + 11.124939d*E
RY    Sct    (JD2414800 - 36100) [00007]; since JD2431200 - see Table.
RY    Sct    The shape of the light curve varies.
RZ    Sct    Min II 7.47. P var. There is nonlinear term in the
RZ    Sct    elements given in the Table: +0.78d*10**(-7)*E**2.
SU    Sct    P var. Max = 2424324.48 + 1.467713d*E (JD2420700 - 34310);
SU    Sct    Max = 2439678.428 + 1.468753d*E (JD2437100 - 41100) [07806];
SU    Sct    since JD2441100 - see Table.
TX    Sct    CWA? red.
TY    Sct    [A/H] = -0.3. In the region of the open cluster Tr 35.
UZ    Sct    [Fe/H] = 0.35. P var. Max = 2435629.5 + 14.7468d*E
UZ    Sct    (JD2423900 - 35700) [02309]; since JD2436000 - see Table.
VV    Sct    SF component of a pair.
VW    Sct    P var. Max = 2415887 + 234d*E (JD2411900 - 22210);
VW    Sct    Max = 2423588 + 235d*E (JD2422880 - 27600);
VW    Sct    Max = 2429468 + 235.1d*E (JD2428750 - 34200);
VW    Sct    since JD2434600 - see Table.
VX    Sct    d = 0.064P.
VZ    Sct    Min II 12.0.
WY    Sct    P var.
XY    Sct    Min II 14.5.
AC    Sct    d = 0.024P; Min II 10.2.
AE    Sct    d = 0.04P.
AI    Sct    In the region of the open cluster NGC 6705.
AN    Sct    P var?
AP    Sct    V2 (NGC 6712).
AU    Sct    d ~0.03P.
BC    Sct    Following component of a close double system. The
BC    Sct    companion - NSV 11551.
BH    Sct    Min II 14.9.
BI    Sct    VB A (B 16.3m:, 3", 280deg; C 16.7m:, 12", 190deg;
BI    Sct    D 16.8m:, 18", 45deg; E 17.0m:, 6", 350deg).
BK    Sct    Close companion 16.5m sf.
BN    Sct    d = 0.02P.
BP    Sct    S 5.5/5.5.
BS    Sct    Min II 11.07. In the region of the open cluster M11
BS    Sct    (NGC 6705).
BU    Sct    A var. P var. Max = 2425804.625 + 0.42022d*E [01401];
BU    Sct    Max = 2427928.041 + 0.4202188d*E (JD2427900 - 9440)
BU    Sct    [01404]; Max = 2432770.464 + 0.4201944d*E
BU    Sct    (JD2432740 - 38290); Max = 2438589.357 + 0.4202171d*E
BU    Sct    (JD2438580 - 40510) [07806]; since JD2440770 - see Table.
BX    Sct    [A/H] = -0.9.
CD    Sct    Min II 13.7.
CF    Sct    d = 0.035P.
CH    Sct    V7 (NGC 6712). The member of this globular cluster.
CK    Sct    [Fe/H] = 0.23.
CL    Sct    May be the period should be doubled?
CM    Sct    [A/H] = 0.1.
CN    Sct    [A/H] = -1.5.
CO    Sct    P var? Resembles RV Tau type variables: if the period is
CO    Sct    doubled, the neight of max I and the depth of Min II vary.
CR    Sct    Min II 12.1; DII = 0.071P; Min II - Min I = 0.53P.
CT    Sct    Min II 11.1.
CW    Sct    Min II 10.1.
DD    Sct    One of the components probably varies.
DE    Sct    Min II 16.3.
DG    Sct    d = 0.03P:.
DL    Sct    Min II 15.9.
DT    Sct    Min II 16.5.
DV    Sct    Min II 17.8.
DW    Sct    Min II 16.4.
EE    Sct    Min II 15.3.
EH    Sct    Min II 15.0.
EK    Sct    Min II 16.0.
EL    Sct    The shape of the light curve varies?
EN    Sct    Min II 17.2. The different elements are also possible:
EN    Sct    Min I = 2428008.85 + 1.06446d*E.
EP    Sct    d = 0.04P:; Min II 15.6.
EQ    Sct    In the region of the open cluster NGC 6631. Min II 12.6:.
ER    Sct    Min II 9.3; Min II - Min I = 0.506P; DII = 0.14P.
EU    Sct    VB A (B 17.5m, 6", 45deg).
EV    Sct    [A/H] = -0.4. The member of the open cluster NGC 6664.
EW    Sct    P0 = 5.8195d (A/2 = 0.27m), P1 = 4.0646d (A/2 = 0.22m);
EW    Sct    P1/P0 = 0.6984.
EX    Sct    d = 0.025P:.
EY    Sct    Min II 12.4. In the region of the open cluster NGC 6683.
EZ    Sct    Min II 12.5.
FF    Sct    Min II 14.2.
FG    Sct    Min II 14.70. P var? Min I = 2429017.557 + 0.2705728d*E
FG    Sct    (JD2427975 - 29520) [01397]; since JD2444700 - see Table.
FH    Sct    In the region of the open cluster NGC 6694.
FK    Sct    Min II 14.4:.
FL    Sct    Min II 13.8.
FM    Sct    Min II 12.9.
FN    Sct    In the open cluster NGC 6704.
FO    Sct    D = 0.22d.
FR    Sct    Spectrum description [01410].
GI    Sct    Min II 14.5.
GM    Sct    Min II 13.8:.
HI    Sct    D = 0.29d.
HL    Sct    Min II 13.4.
IS    Sct    P < 200d.
IT    Sct    In the region of the open cluster NGC 6705.
LL    Sct    sf component of a close pair.
LR    Sct    V14 (NGC 6712).
LU    Sct    P2 = 30d.
LZ    Sct    In the region of the globular cluster NGC 6712.
MM    Sct    Min II 15.8.
MP    Sct    V1 (NGC 6712). The member of this globular cluster.
MP    Sct    [Fe/H] = -0.69.
MR    Sct    V8 (NGC 6712). P var. Max = 2430885 + 117d*E
MR    Sct    (JD2427900 - 32400) [04231]; since JD2434900 - see Table.
NU    Sct    VB A (B 16.6m, 12", 180deg).
NV    Sct    P = 200d?
OU    Sct    P var. Max = 2427620 + 152d*E (JD2426200 - 32800);
OU    Sct    since JD2433100 - see Table.
PT    Sct    There is a close companion, 16.4m.
PW    Sct    The range of the combined light of the variable and
PW    Sct    a close companion, which follows, is given in the Table.
QU    Sct    The variable is also eclipsing one with P = 0.2d and
QU    Sct    A = 0.7m.
V0337 Sct    A close companion (16.2m, <7", 90deg).
V0340 Sct    Min II 15.6.
V0356 Sct    Min II 12.3; DII = 0.10P.
V0360 Sct    A close fn companion, 16.4m.
V0362 Sct    P = 170d?
V0367 Sct    In the open cluster NGC 6649. The light elements
V0367 Sct    with fundamental mode period P0 (A0 = 0.54m B) are
V0367 Sct    given in the Table. For the first-overtone period
V0367 Sct    P1 (A1 = 0.41m B) Max = 2437435.12 + 4.38466d*E;
V0367 Sct    P1/P0 = 0.696744. M - m var (0.15 <= M - m <= 0.45).
V0369 Sct    In the region of the open cluster NGC 6705 (M 11).
V0369 Sct    There is a superposition of the four light oscillations:
V0369 Sct    P1 = 0.240d (A1 = 0.044m), P2 = 0.220d (A2 = 0.020m),
V0369 Sct    P3 = 0.182d (A3 = 0.068m), P4 = 0.114d (A4 = 0.028m)
V0369 Sct    [09745].
V0370 Sct    d = 0.016P.
V0372 Sct    d = 0.012P.
V0414 Sct    Blue companion?
V0479 Sct    Porb = 4.4267 d.
V0484 Sct    MinII 9.22.
V0490 Sct    Min II 13.6; Min II - Min I = 0.326P; DII = 0.025P.
V0491 Sct    Min II 14.1.
V0493 Sct    MinII - MinI = 0.75P.
V0498 Sct    Multiperiodic.
del   Sct    VB A (B 10m, 53", 130deg); (k - b)2 = 0.37.
del   Sct    The basic light variation P0 (A0 = 0.125m) given in the
del   Sct    Table is superposed by the secondary one with
del   Sct    P1 = 0.1867756 (A1 = 0.034) [09975].
R     Ser    P var. Max = 2372429 + 356.93d*E (JD2372400 - 88900)
R     Ser    [00960]; Max = 2397809 + 353.00d*E
R     Ser    (JD2394000 - 2403000); Max = 2403104 + 357.25d*E
R     Ser    (JD2403000 - 24000); Max = 2432387 + 356.10D*E
R     Ser    (JD2424000-39200); since JD2441000 - see Table.
R     Ser    Maser (SiO, H2O).
S     Ser    P var. Max = 2394360 + 361.01d*E (JD2394000 - 2407000);
S     Ser    Max = 2407024 + 372.70d*E (JD2407000 - 17000) [00960];
S     Ser    Max = 2425875 + 366.59d*E (JD2417000 - 36000); since
S     Ser    JD2437600 - see Table. Maser (OH, SiO, H2O).
T     Ser    In the region of the open cluster NGC 6633.
T     Ser    P var. Max = 2400907 + 342.05d*E (JD2400500 - 15000);
T     Ser    Max = 2417912 + 345.73d*E (JD2417900 - 26000);
T     Ser    Max = 2428524 + 332.21d*E (JD2426000 - 32500);
T     Ser    Max = 2438382 + 345.71d*E (JD2432500 - 39500); since
T     Ser    JD2439500 - see Table. 0.8' from BN Ser.
U     Ser    P var. Max = 2421158 + 237.70d*E (JD2414000 - 22000);
U     Ser    Max = 2422347 + 236.78d*E (JD2422000 - 26600);
U     Ser    Max = 2426609 + 239.21d*E (JD2426600 - 32500);
U     Ser    since JD2432500 - see Table.
V     Ser    Min II 9.85.
W     Ser    P var, nonlinear terms:
W     Ser    +(3.140d*10**(-6))*E**2 + (1.432d*10**(-9))*E**3.
W     Ser    The light curve shape var. Wavelike variations in Max
W     Ser    light. Changes of emission lines with the orbital phase.
W     Ser    Active mass exchange, evidence for a common envelope.
X     Ser    After 1932 variations 14.3m - 18.3m were noted; according
X     Ser    to [01417], P = 275d. Observations in 1961 - 1964 did not
X     Ser    confirm P = 275d, fluctuations of light with a period of
X     Ser    several minutes were suspected [03625]. The spectral data
X     Ser    are for 1981.
Y     Ser    Epoch of min is given. According to [08643], variations
Y     Ser    with P ~400d are superimposed by P ~40d.
Z     Ser    The elements are valid during JD2422000 - 31000.
RS    Ser    Min II 11.4.
RT    Ser    Max (1920 - 1923). In the spectrum (1977 - 1979) there are
RT    Ser    emissions Halpha - Hdelta, HeI, HeII, [OI] etc.
RT    Ser    Absorptions TiO.
RV    Ser    Maser (H2O).
VY    Ser    [Fe/H] = -1.77, Delta(S) = 9.
WW    Ser    Maser (H2O).
WX    Ser    Maser (OH, SiO, H2O). P var?
AA    Ser    [A/H] = 0.2.
AG    Ser    P var? since JD2435000 - see Table.
AK    Ser    P var? before JD2442300 Min = 2431313.266 + 1.9225667d*E
AK    Ser    [00318]; since JD2442300 - see Table.
AN    Ser    P var? Max = 2429156.260 + 0.5220703d*E
AN    Ser    (JD2427000 - 38000) [00001]; since JD2438000 - see Table.
AN    Ser    According to [02740], Blazhko effect with Pi = 21.94d;
AN    Ser    the presence of the Blazhko effect is denied in [07258].
AN    Ser    Delta(S) = 0.
AO    Ser    Min II 10.8.
AP    Ser    VB A (B 14.29m, 8" sp). [Fe/H] = -1.37.
AQ    Ser    Min II 11.1.
AR    Ser    P var. Before JD2425000 Max = 2415617.698 + 0.5752221d*E;
AR    Ser    Max = 2425313.530 + 0.57508945d*E
AR    Ser    (JD2425000 - 28500); Max = 2428848.662 + 0.575214d*E
AR    Ser    (JD2428500 - 31000) [08081]; Max =
AR    Ser    2431436.424 + 0.5751134d*E (JD2431000 - 34200);
AR    Ser    Max = 2436013.279 + 0.5752169d*E (JD2435900 - 37200);
AR    Ser    Max = 2438138.467 + 0.5750651d*E (JD2437200 - 38700)
AR    Ser    [00001]. Elements working on average since JD2438700 - see
AR    Ser    Table. Complex Blazhko effect. Pi = 108.4d [08082].
AR    Ser    A var (0.23m - 0.87m V). Pi var (80d - 120d) [07032].
AR    Ser    Delta(S) = 4.6.
AS    Ser    Min II 11.5. The epoch of Min I 2442937.428
AS    Ser    (BBSAG) is not in agreement with the elements.
AT    Ser    P var. Max = 2415353.783 + 0.74655695d*E
AT    Ser    (JD2415000 - 27000); Max = 2428337.260 + 0.7465670d*E
AT    Ser    (JD2428000 - 39500); since JD2441500 - see Table.
AT    Ser    Delta(S) = 9.
AU    Ser    Min II 11.61.
AU    Ser    The light curve shape var.
AV    Ser    Delta(S) = 6.
AW    Ser    Delta(S) = 5.0.
BF    Ser    [A/H] = -2.5. Delta(S) = 6.
BH    Ser    P var. Max = 2427956.674 + 0.434545d*E (JD2425000 -
BH    Ser    30700) [01039]; since JD2437650 - see Table.
BI    Ser    Min I 2446264.414 [10200] contradicts the elements. P var?
BN    Ser    In the region of the open cluster NGC 6633. 0.8' from
BN    Ser    T Ser.
BO    Ser    P var? Max = 2425681 + 201d (JD2425600 - 30100)  0447];
BO    Ser    the Table gives mean elements (JD2425600 - 35400).
BQ    Ser    P0 - see Table. P1 = 3.012d [08188]. In the region of the
BQ    Ser    open cluster IC 4756.
BR    Ser    In the region of the open cluster IC 4756.
BS    Ser    In the region of the open cluster IC 4756.
BT    Ser    In the region of the open cluster IC 4756.
BU    Ser    In the region of the open cluster IC 4756.
CC    Ser    Min II 11.63.
CN    Ser    [Fe/H] = -0.77. Delta(S) = 3.4.
CO    Ser    P var? The light curve shape var.
CO    Ser    [Fe/H] = -1.38. Delta(S) = 7.2.
CQ    Ser    Min II 12.0.
CR    Ser    [A/H] = -0.2.
CS    Ser    P var. Max = 2418137.875 + 0.5267904d*E
CS    Ser    (JD2416000 - 32500) [00001]; since JD2432500 - see Table.
CS    Ser    Delta(S) = (6). In the region of the HII complex S 54 and
CS    Ser    the open star cluster NGC 6604. Connected with a
CS    Ser    shell-structure nebula. Sometimes eclipses are observed
CS    Ser    during the configuration "WR in front of O" (see Table)
CS    Ser    and sometimes during the configuration "O in front of
CS    Ser    WR" which coincided with the deepest eclipse ever observed
CS    Ser    (with the depth 0.5m B, V). Sometimes the photometric
CS    Ser    eclipse at predicted moments does not occur, and only the
CS    Ser    atmospheric eclipse of the O star with the WR component is
CS    Ser    observed at lambda 4653 A (emission of CII - CIV, NIII),
CS    Ser    lambda < 2000 A. IR excess; possibly an IR eclipse in
CS    Ser    the configuration "O  in front of WR".
CX    Ser    The light curve (resembling the eclipsing light curve of
CX    Ser    U Gem) shows a hump of ~0.2m height before the minimum;
CX    Ser    fluctuations up to ~0.3m - 0.4m in Max.
DF    Ser    VB A (B 13.9m, 0.4', -115deg).
DG    Ser    Min II 16.5:. The alias period is possible (0.3360742d).
DH    Ser    Another possible P = 450d.
DK    Ser    Max 2433829 [10008] contradicts the elements.
DR    Ser    VB A (B 12.54m, 28", 0deg).
DT    Ser    VB A (B ~5"). The spectrum shows emissions of [OIII]
DT    Ser    lambda lambda 4959, 5007 A. Symbiotic? [08676].
DV    Ser    In a small star cluster.
DY    Ser    [Fe/H] = -1.58. Delta(S) = 8.4.
EE    Ser    In the region of the open cluster M 17 = NGC 6618.
EF    Ser    In the region of the open cluster M 17 = NGC 6618.
EG    Ser    VB A (ro > 10").
EL    Ser    N <= 7.
EN    Ser    [Fe/H] = -1.07. Delta(S) = 5.3.
EO    Ser    The light curve shows large scatter. RR(B) type is
EO    Ser    possible. Max = 2437433.653 + 0.6309d*E (JD2437433 - 514)
EO    Ser    [3625]. [Fe/H] = -1.63. Delta(S) = 8.8.
ER    Ser    In the region of the open cluster M 16 = NGC 6611.
ES    Ser    In the region of the open cluster M 16 = NGC 6611.
ET    Ser    In the region of the open cluster M 16 = NGC 6611.
EU    Ser    VB A (B 4" np). A member of the open cluster
EU    Ser    M 16 = NGC 6611. IR excess.
EV    Ser    In the region of the open cluster M 16 = NGC 6611.
EW    Ser    In the region of the open cluster M 16 = NGC 6611.
EX    Ser    In the region of the open cluster M 16 = NGC 6611.
FI    Ser    Hints of periodicity in U light.
FK    Ser    VB (Delta(m) ~0.5m, 1.3", 11.5deg, 1972).
FK    Ser    Flares were found in the satellite UV range [10013].
FK    Ser    Differences from typical by stars and probable "post-T Tau"
FK    Ser    nature are noted [07260, 03866]. According to [06948],
FK    Ser    Min = 2441939.200 + 5.20d*E. Soft X-ray source.
FL    Ser    VB (Delta(m) = 1.9m, 0.46", 145deg, 1981).
FM    Ser    In the region of the open cluster M 16 = NGC 6611.
FM    Ser    VB (var sf?).
FN    Ser    In the region of the open cluster M 16 = NGC 6611.
FR    Ser    ADS 11477 A (B 12.5m, 10.5", 330deg, 1924; C 9.3m,
FR    Ser    30.5", 5deg, 1930). Possible values of P: 2.1308d, 2.1565d.
LN    Ser    m pg ~17.5m ~const; blue companion? [07264].
LS    Ser    The light curve shows large scatter, the elements need
LS    Ser    confirmation. Possible identification with an X-ray source
LS    Ser    2ASE 1822 + 0.
LV    Ser    The epoch of max in V light is given; in B and U varies
LV    Ser    in opposite phase.
LX    Ser    The depth of eclipses ~2.5m. Comparatively frequent
LX    Ser    outbursts [10023].
MM    Ser    Ser X-1 = 4 U 1 837 + 04. LX/Lopt >= 100.
MM    Ser    VB B (A 19.1m; B 2.2", 210deg).
MO    Ser    V1 (NGC 6535). Cluster non-member.
MP    Ser    V2 (NGC 6535). Cluster non-member.
OU    Ser    SB2.
PS    Ser    Both components are SB systems, Porb(A) = 15.888d,
PS    Ser    Porb(B) = 13.561d.
PT    Ser    SB, Porb = 38.937d.
V0381 Ser    SB2.
V0383 Ser    SB2.
V0384 Ser    MinII 12.35.
V0391 Ser    The coordinates in [230] are wrong.
V0393 Ser    VB A (B 15" np).
V0399 Ser    MinII 11.9.
V0413 Ser    Apsidal motion, P(MinII) = 2.259735d. VB(9.1m, 9.1m, 0.3", 215deg, 1991).
V0425 Ser    Min II = 12.1.
V0437 Ser    Superposed variations with an amplitude about 0.3m and a period of 44d.
V0462 Ser    P = 0.274277d is also possible.
V0466 Ser    P = 0.177978d is also possible.
V0493 Ser    Porb = 0.07408d, superhumps: P = 0.082866d.
V0497 Ser    P = 0.302612d is also possible.
V0499 Ser    Multiperiodic.
V0501 Ser    P = 0.266086d is also possible.
V0539 Ser    Multiperiodic.
del   Ser    ADS 9701A (B 5.16m, dF0, a = 5.843", Porb = 3168 yr;
del   Ser    4", 175G, 1980).
omi   Ser    SB?
d     Ser    ADS 11353 A (B 7.44m, SB?, F5V, 3.9", 320deg, 1983).
d     Ser    VB (speckle-interferometric; 0.25", 157deg, 1976).
d     Ser    SB (P1orb = 385d, P2orb = 1.8505205d).
S     Sex    P var. Max = 2422029 + 257.2d*E (JD2417650 - 22050);
S     Sex    Max = 2428968 + 266.65d*E (JD2422050 - 30300); Max =
S     Sex    2434739 + 260.86d*E (JD2430300 - 34750); Max =
S     Sex    2438796 + 254.3d*E (JD2434750 - 38800);
S     Sex    since JD2440600 - see Table.
T     Sex    [Fe/H] = -1.20. P var. Max = 2416146.675 + 0.32465971d*E
T     Sex    (JD2414000 - 18300), Max = 2424561.398 + 0.32467107d*E
T     Sex    (JD2418300 - 24570) [00752];
T     Sex    Max = 2424561.430 + 0.3246702d*E (JD2424560 - 28280),
T     Sex    Max = 2429350.320 + 0.3247113d*E (JD2429350 - 34370),
T     Sex    Max = 2434795.409 + 0.3246978d*E (JD2434795 - 36630)
T     Sex    [09978]; since JD2441380 - see Table.
U     Sex    P var. Max = 2419823.355 + 0.53402622d*E
U     Sex    (JD2419470 - 36670) [03697]; since JD2443980 - see Table.
Y     Sex    Min II 10.17; dII = 0.05P. P var. Min I = 2428122.700 +
Y     Sex    0.41982341d*E (JD < 2429000) [00007]; Min I =
Y     Sex    2434445.989 + 0.419818d*E (JD2428100 - 35000)
Y     Sex    [00001], Min I = 2439521.964 + 0.41981543d*E
Y     Sex    (JD2431150 - 43250) [09981]; since JD2440300 - see Table.
RU    Sex    Min II 11.4. According to [09923], RR?
RU    Sex    (P = 0.5398d?), CEP? (P = 6.792d?).
RW    Sex    Porb = 0.247d [09925]; LX/Lopt = 10**(-4) [09926];
RW    Sex    Px = 254s [09927].
RX    Sex    VB A (B 9.1m, 116.3", 191deg).
RY    Sex    Mu = 0.67", P = 281deg.
WW    Sex    MinII 10.46.
WX    Sex    MinII 12.8.
WY    Sex    The depth of MinII is 0.29.
WZ    Sex    MinII 10.0.
AI    Sex    Min II = 11.0.
AO    Sex    P = 0.234675d is also possible.
AY    Sex    A millisecond radio pulsar showing optical variations with the tabulated orbital period. Dramatic shanges in the spectrum were recorded.
BG    Sex    P = 0.415502d is also possible.
BP    Sex    VB A (B 10.96mV, 1.3", 342deg, 1991).
R     Tau    OH, H2O, Sio maser. P var. Max = 2411012 +
R     Tau    325.0d*E (JD2398654 - 2414000); Max = 2424243 +
R     Tau    322.1d*E (JD2414000 - 24300); Max = 2434005 +
R     Tau    325.4d*E (JD2424300 - 35500); since JD2435500 - see Table.
S     Tau    P var. Max = 2404646 + 380.1d*E (JD2399326 - 2405000);
S     Tau    Max = 2425085 + 371.40d*E (JD2405000 - 26000); since
S     Tau    JD2426000 - see Table.
T     Tau    VB A (B 15m, 0.27", 358deg; C - infrared companion, 0.590",
T     Tau    180deg). Near the variable nebula NGC 1555. OH, H2O maser.
T     Tau    In the interval JD2402140 - 21000 the light range
T     Tau    9.3m - 13.5m, since JD2421000 - only 9.5m - 10.8m.
U     Tau    VB (A 10.9m; B 12.0m, 3", 77deg).
V     Tau    P var. Max = 2417978 + 170.0d*E (JD2404550 - 18000);
V     Tau    Max = 2424580 + 169.3d*E (JD2418000 - 24600);
V     Tau    Max = 2432746 + 170.1d*E (JD2424600 - 33500);
V     Tau    Max = 2436970 + 168.7d*E (JD2433500 - 37300);
V     Tau    Max = 2442442 + 171.1d*E (JD2437300 - 43000);
V     Tau    since JD2443000 - see Table.
W     Tau    P value is given in the Table.
W     Tau    P var. Max = 2415320 + 274.1d*E (JD2410360 - 15500),
W     Tau    Max = 2421995 + 266.1d*E (JD2415500 - 22500),
W     Tau    Max = 2425135 + 260.5d*E (JD2422500 - 28800),
W     Tau    Max = 2438837 + 245.4d*E (JD2428800 - 39100) [00001].
Z     Tau    VB A (B 13.6m, 4", 45deg).
Z     Tau    P var. Max = 2425115 + 499.90d*E (JD2415100 - 26500)
Z     Tau    Max = 2438768 + 486.20d*E (JD2426500 - 39000);
Z     Tau    since JD2439000 - see Table.
RR    Tau    Spectrum description and the photographs of the nebula
RR    Tau    [04002].
RU    Tau    VB A (B 4"). P var. Max = 2426004 + 545.3d*E
RU    Tau    (JD2415009 - 27500). Max = 2434309 + 604.0d*E
RU    Tau    (JD2427500 - 34500); since JD2437500 - see Table.
RV    Tau    OH maser. Mean brightness varies: Min = 2417553 + 1224d*E
RV    Tau    [00580].
RW    Tau    VB A (12.5m, 1.3", 172deg, 1959). dI = 0.020P; Min II 8.09.
RW    Tau    P var. Min I = 2417198.410 + 2.7688665d*E +
RW    Tau    0.038d*sin(0.0818deg*(E - 100)) (JD2409913 - 24150),
RW    Tau    Min I = 2434423.3571 + 2.7688209d*E (JD2424150 - 37000)
RW    Tau    [05460]; Min I = 2437164.4860 + 2.7688480d*E
RW    Tau    (JD2437000 - 39900) [07531]; Min I = 2442776.93772 +
RW    Tau    2.76884463d*E (JD2439855 - 42780) [08593]; Min I =
RW    Tau    2442776.9313 + 2.7688396d*E (JD2442780 - 45750)
RW    Tau    [09084]; since JD2445750 - see Table. The shape of the
RW    Tau    light curve varies.
RX    Tau    OH, H2O maser. P var. Max = 2423561 + 338.4d*E
RX    Tau    (JD2417155 - 24000); Max = 2430505 + 330.2d*E
RX    Tau    (JD2424000 - 30700); Max = 2437963 + 339.3d*E
RX    Tau    (JD2430700 - 38000); since JD2438000 - see Table.
RY    Tau    SB1. The photographs of the nebula and spectrum
RY    Tau    description [05064]. Long period light variations are
RY    Tau    possible with cycles 70.25, 15.9, 9.4 and 5.84 years
RY    Tau    [09993].
RZ    Tau    Min II 10.66. P var. Min I = 2424032.1426 +
RZ    Tau    0.41567109d*E (JD2424000 - 34100) [00312];
RZ    Tau    since JD2436000 - see Table.
SS    Tau    P var [03506]. Max = 2420894.2339 + 0.3699665d*E
SS    Tau    (JD2420890 - 21300) [09995]; Max = 2426669.080 +
SS    Tau    0.3699687d*E (JD2426400 - 26700) [00320]; Max =
SS    Tau    2428843.856 + 0.3699231d*E (JD2426700 - 30300),
SS    Tau    Max = 2431392.603 + 0.369912d*E (JD2430300 - 31400),
SS    Tau    Max = 2432118.794 + 0.369937d*E (JD2431400 - 32150),
SS    Tau    Max = 2432857.884 + 0.3699146d*E (JD2432150 - 35000),
SS    Tau    Max = 2435055.528 + 0.3699066d*E (JD2435000 - 36400),
SS    Tau    Max = 2437313.503 + 0.3699266d*E (JD2436400 - 37320),
SS    Tau    Max = 2437960.419 + 0.369878d*E (JD2437300 - 37960),
SS    Tau    Max = 2437960.419 + 0.369938d*E (JD2437960 - 38740);
SS    Tau    since JD2438740 - see Table.
SV    Tau    Min II 9.8.
SW    Tau    P var. Max = 2432049.856 + 1.583623d*E (JD2418240 - 36000);
SW    Tau    since JD2436000 - see Table.
SX    Tau    In the region of the Pleiades cluster. Not a member
SX    Tau    of the cluster.
SY    Tau    In the region of the Pleiades cluster. Not a member
SY    Tau    of the cluster.
SZ    Tau    The member of the halo of the open cluster NGC 1647.
SZ    Tau    P var. Max = 2410000.60 + 3.1487d*E (JD2412000 - 20200)
SZ    Tau    [09996]; Max = 2419267.519 + 3.149046d*E
SZ    Tau    (JD2419260 - 34650); since JD2434650 - see Table.
TT    Tau    P = 364d? [00589].
TY    Tau    In the region of the hyades cluster. Not a member of
TY    Tau    the cluster. According to [09997], Min = 2422291.303 +
TY    Tau    0.539250d*E.
UU    Tau    In the region of the Pleiades cluster. Not a member of
UU    Tau    the cluster.
UX    Tau    VB A (B 13.67m V, M2.5 VE, 5.74", 270.1deg, 1944).
UZ    Tau    VB A (B 15.16m B, M4VE (Li), 3.7", 271.5deg, 1944).
UZ    Tau    The range of the combined light variation is given in the
UZ    Tau    Table.
VW    Tau    The chart in [06286] is wrong.
WW    Tau    P var. P = 114.8d (JD2414800 - 20800). P = 124.4d
WW    Tau    (JD2420800 - 23700) [00634]; P = 114d (JD2424800 - 26300),
WW    Tau    P = 139d (JD2426300 - 27700) [00310]; P = 114d
WW    Tau    (JD2427900 - 30800), P = 131d (JD2430800 - 31500),
WW    Tau    P = 109d (JD2431500 - 33400) [00364]; since
WW    Tau    JD2433400 - see Table.
WY    Tau    Min II 11.73. P var? [10048].
WZ    Tau    VB.
XZ    Tau    VB A (B = HL Tau, 23", 273deg).
YZ    Tau    [Fe/H] = -1.53. In the region of the Pleiades cluster.
YZ    Tau    Not a member of the cluster.
YZ    Tau    There is a square term in the elements: -6d*10**(-11)*E**2.
AA    Tau    Cyclic light variation with P = 4.5d and 2d [10003] and
AA    Tau    also 8.2d [10004] is possible.
AC    Tau    d = 0.025P. P var?
AH    Tau    Min II 11.85. P var? In the region of the Pleiades
AH    Tau    cluster. Not a member of the cluster.
AL    Tau    P var. The depth of Min II 0.15m.
AM    Tau    d = 0.012P:. P var. Min I = 2427534.444 + 2.044018d*E
AM    Tau    (JD2425580 - 27540), Min I = 2435019.436 +
AM    Tau    2.043935d*E (JD2433320 - 37020); since JD2442365 - see
AM    Tau    Table.
AN    Tau    Min II 10.5; Min II - Min I = 0.53P. P var.
AP    Tau    Min II 14.7; Min II - Min I = 0.48P.
AS    Tau    P var. Min I = 2439390.595 + 3.4835542d*E
AS    Tau    (JD2419440 - 44300) [07806]; since JD2444300 - see Table.
AU    Tau    P var. Max = 2426642 + 71.0d*E (JD2426290 - 30400)
AU    Tau    [00310]; since JD2438000 - see Table.
AW    Tau    OH, H2O maser. P var. Max = 2426278 + 690d*E
AW    Tau    (JD2416100 - 33850) [00609]; since JD2433850 - see Table.
BB    Tau    SC 7/7 e.
BK    Tau    In the region of the Pleiades cluster. Not a member of
BK    Tau    the cluster.
BN    Tau    P var. Min I = 2435460.370 + 4.2542044d*E
BN    Tau    (JD2419000-39100) [05466]; since JD2443000 - see Table.
BP    Tau    There are quasisinusoidal light variations with P = 7.6d
BP    Tau    [10011].
BU    Tau    Pleione. The member of the Pleiades cluster.
BV    Tau    Min II 11.9.
BW    Tau    3C 120. Seyfert galaxy; Z = 0.033. Spectrum description
BW    Tau    [10012].
CD    Tau    VB A (B 9.88m, 9.9", 148.8deg). Min II 7.31.
CD    Tau    In the region of the open cluster CR 65.
CF    Tau    d = 0.02P; Min II 10.2;
CH    Tau    The epoch of Min brightness is given.
CM    Tau    SN 1054 in the Crab nebula (NGC 1952 = M1); pulsar NP 0532.
CM    Tau    The outburst epoch is JD2106210:. The pulsed radiation
CM    Tau    varies precisely in phase over the whole spectrum, from
CM    Tau    radio waves to gamma rays with P = 0.033S in the range
CM    Tau    13.9m - 17.7m V. P var [10017, 10018]: 0.033095563927s
CM    Tau    (JD2440297.5094) <= P <= 0.033242051159s (JD2444312.750).
CR    Tau    P = 1.362692d?
CT    Tau    Min II 11.12. P var. Min I = 2437312.369 + 0.6668274d*E
CT    Tau    (JD2432700 - 38790) [10010]; since JD2441400 - see Table.
CU    Tau    In the region of the Pleiades cluster. Not a member of
CU    Tau    the cluster. Min II 11.90. P var. Min I =
CU    Tau    2431822.5193 + 0.4126022d*E (JD2431060 - 2890)
CU    Tau    [00604]; since JD2440960 - see Table.
CZ    Tau    VB B (A = DD Tau; B 31", 13deg).
DD    Tau    VB A (B = CZ Tau; 31", 13deg.
DE    Tau    VB A (B 26", 10deg).
DG    Tau    Connected with a small bright arc-shaped nebula.
DH    Tau    VB A (B = DI Tau, 16", 125deg). According to [10004] there
DH    Tau    is periodical light variability with P = 7.0d and
DH    Tau    A = 0.4m V.
DI    Tau    VB B (A = DH Tau; B 16", 125deg).
DI    Tau    According to [10004] there is
DI    Tau    periodical light variability with P ~7.0d and A < 0.4m V.
DL    Tau    VB A (B 17m V, 12", 333deg).
DL    Tau    Cyclic light variation with P = 2.7d is present [10003].
DN    Tau    There are sinusoidal light variations with
DN    Tau    P = 6.6d [10011].
DO    Tau    Connected with a small bright arc-shaped nebula.
DS    Tau    VB A (B 13.7m, 4", 288deg). Range of Combined light
DS    Tau    variation of the pair is given in the Table.
EI    Tau    VB?
EQ    Tau    Min II 10.97. In the region of the Pleiades cluster.
EQ    Tau    Not a member of the cluster.
ET    Tau    Min II 9.3.
EY    Tau    The member of the Hyades cluster.
EZ    Tau    The member of the Hyades cluster.
FH    Tau    The member of the Hyades cluster.
FL    Tau    The member of the Pleiades cluster.
FS    Tau    VB A (B 16", 289deg).
FV    Tau    VB A (B 13", 103deg).
FW    Tau    VB A (B 13", 243deg).
FY    Tau    VB B (A = FZ Tau, B 17", 250deg.)
FZ    Tau    VB A (B = FY Tau, 17", 250deg).
GG    Tau    VB A (B 18.5m, 12", 205deg).
GH    Tau    VB B (A = V807 Tau; B 21.4", 193deg).
GI    Tau    VB B (A = GK Tau; B 13", 329deg). There are
GI    Tau    quasisinusoidal light variations with P = 7.2d [10011].
GI    Tau    Connected with a small bright arc-shaped nebula.
GK    Tau    VB A (B = GI Tau, 13", 329deg).
GK    Tau    There are quasisinusoidal light variations with P = 4.6d
GK    Tau    [10011]. Connected with a small bright arc-shaped nebula.
GL    Tau    The central star of the planetary nebula PK 174 -14deg 1.
GP    Tau    P2 = 1000d.
GR    Tau    dI = 0.068P; Min II 10.49; Mim II - Min I = 0.516P.
GS    Tau    SB1 (Porb = 7.227424d [06568]). The epoch of Min
GS    Tau    brightness is given.
GU    Tau    VB A (B 11", 299deg).
GV    Tau    Herbig-haro object.
GW    Tau    Min II 11.7. P var?
GX    Tau    VB A (B 11", 310deg).
HK    Tau    VB A (B 21m, 2", 180deg).
HL    Tau    VB B (A = XZ Tau; B 23", 273deg). Connected with a
HL    Tau    small bright arc-shaped nebula.
HN    Tau    VB A (B 18m, 3.3", 205deg).
HO    Tau    VB A (B 8", 110deg).
HP    Tau    Connected with a small bright arc-shaped nebula.
HP    Tau    According to [10004] there is periodical variability
HP    Tau    with P = 1.2d.
HR    Tau    VB B (A = HS Tau; B 14", 119deg).
HS    Tau    VB A (B = HR Tau; 14", 119deg).
HU    Tau    Min II 5.91.
HW    Tau    Minor planet (49) Pales.
HZ    Tau    In the region of the Pleiades cluster. Possible
HZ    Tau    member of the cluster.
II    Tau    In the region of the Pleiades cluster.
II    Tau    Possible member of the hyades cluster
IK    Tau    OH, H2O, SiO maser.
IM    Tau    P var. Max = 2439792.398 + 0.144969d*E (JD2439790 -
IM    Tau    43130) [10019]; P1 = 0.109016d, P1/P0 = 0.752.
IM    Tau    Since JD2444230 - see Table.
IN    Tau    mu = 0.121", P = 105deg. The member of the Hyades cluster?
IO    Tau    In the region of the Hyades cluster.
IQ    Tau    VB A (B 17m, 11", 298deg).
IS    Tau    SVS 1319 [04051].
IS    Tau    The star N23 with Halpha emission [00596]. In the map given
IS    Tau    in [00596] erroneously designated as N26 in contradiction
IS    Tau    with the co-ordinates given in the same paper. It was the
IS    Tau    reason for different mistakes when the
IS    Tau    star was identified by some other investigators.
IT    Tau    SVS 1320 [04051].
IT    Tau    The star N26 with Halpha emission [00596].
IT    Tau    In the map given in [00596] IS Tau erroneously designated
IT    Tau    as N26 in contradiction with the co-ordinates given in the
IT    Tau    same paper. It was the reason for different mistakes when
IT    Tau    IS Tau was identified by some other investigators.
KK    Tau    In the region of the Pleiades cluster.
KL    Tau    In the region of the Pleiades cluster.
KM    Tau    In the region of the Pleiades cluster.
KN    Tau    In the region of the Pleiades cluster.
KO    Tau    In the region of the Pleiades cluster.
KP    Tau    In the region of the Pleiades cluster. Not a member
KP    Tau    of the cluster.
KQ    Tau    In the region of the Pleiades cluster.
KR    Tau    In the region of the Pleiades cluster. Not a member
KR    Tau    of the cluster.
KS    Tau    In the region of the Pleiades cluster.
KT    Tau    In the region of the Pleiades cluster.
KU    Tau    In the region of the Pleiades cluster.
KV    Tau    In the region of the Pleiades cluster.
KW    Tau    In the region of the Pleiades cluster.
KX    Tau    In the region of the Pleiades cluster. Not a member
KX    Tau    of the cluster.
KY    Tau    The member of the Pleiades cluster.
KZ    Tau    In the region of the Pleiades cluster.
LL    Tau    In the region of the Pleiades cluster.
LM    Tau    In the region of the Pleiades cluster. Possible member
LM    Tau    of the cluster.
LN    Tau    In the region of the Pleiades cluster.
LO    Tau    In the region of the Pleiades cluster. Possible member
LO    Tau    of the cluster.
LP    Tau    In the region of the Pleiades cluster. Not a member
LP    Tau    of the cluster.
LQ    Tau    In the region of the Pleiades cluster.
LR    Tau    In the region of the Pleiades cluster. Possible member
LR    Tau    of the Hyades cluster.
LS    Tau    In the region of the Pleiades cluster.
LT    Tau    In the region of the Pleiades cluster. Possible member
LT    Tau    of the cluster.
LU    Tau    In the region of the Pleiades cluster. Possible member
LU    Tau    of the cluster.
LV    Tau    In the region of the Pleiades cluster. Possible member
LV    Tau    of the cluster.
LW    Tau    In the region of the Pleiades cluster. Not a member
LW    Tau    of the cluster.
LX    Tau    In the region of the Pleiades cluster.
LY    Tau    In the region of the Pleiades cluster. Possible member
LY    Tau    of the cluster.
LZ    Tau    The member of the Pleiades cluster.
MM    Tau    The member of the Pleiades cluster.
MN    Tau    In the region of the Pleiades cluster.
MO    Tau    In the region of the Pleiades cluster. Possible member
MO    Tau    of the cluster.
MP    Tau    In the region of the Pleiades cluster.
MQ    Tau    In the region of the Pleiades cluster.
MR    Tau    The member of the Pleiades cluster.
MS    Tau    The member of the Pleiades cluster.
MT    Tau    In the region of the Pleiades cluster. Not a member
MT    Tau    of the  cluster.
MU    Tau    In the region of the Pleiades cluster. Possible member
MU    Tau    of the cluster.
MV    Tau    In the region of the Pleiades cluster. Possible member
MV    Tau    of the cluster.
MW    Tau    In the region of the Pleiades cluster.
MX    Tau    The member of the Pleiades cluster.
MY    Tau    The member of the Pleiades cluster.
MZ    Tau    In the region of the Pleiades cluster. Possible member
MZ    Tau    of the cluster.
NN    Tau    In the region of the Pleiades cluster.
NO    Tau    In the region of the Pleiades cluster.
NP    Tau    The member of the Pleiades cluster.
NQ    Tau    In the region of the Pleiades cluster.
NR    Tau    In the region of the Pleiades cluster. Not a member
NR    Tau    of the cluster.
NS    Tau    In the region of the Pleiades cluster.
NT    Tau    In the region of the Pleiades cluster. Possible member
NT    Tau    of the cluster.
NU    Tau    In the region of the Pleiades cluster.
NV    Tau    In the region of the Pleiades cluster. Not a member
NV    Tau    of the cluster.
NW    Tau    In the region of the Pleiades cluster.
NX    Tau    In the region of the Pleiades cluster. Not a member
NX    Tau    of the cluster.
NY    Tau    In the region of the Pleiades cluster. Not a member
NY    Tau    of the cluster.
NZ    Tau    In the region of the Pleiades cluster.
OO    Tau    In the region of the Pleiades cluster.
OP    Tau    In the region of the Pleiades cluster. Possible member
OP    Tau    of the cluster.
OQ    Tau    In the region of the Pleiades cluster.
OR    Tau    The member of the Pleiades cluster.
OS    Tau    The member of the Pleiades cluster.
OT    Tau    The member of the Pleiades cluster.
OU    Tau    Max = 2444896.758 + 0.39701d*E, M - m = 0.5P, A(V) =
OU    Tau    0.13m [10052].
OU    Tau    The member of the Pleiades cluster.
OW    Tau    The member of the Pleiades cluster.
OX    Tau    In the region of the Pleiades cluster.
OY    Tau    In the region of the Pleiades cluster. Not a member
OY    Tau    of the cluster.
OZ    Tau    In the region of the Pleiades cluster. Possible member
OZ    Tau    of the cluster.
PP    Tau    In the region of the Pleiades cluster. Possible member
PP    Tau    of the cluster.
PQ    Tau    In the region of the Pleiades cluster. Not a member
PQ    Tau    of the cluster.
PR    Tau    The member of the Pleiades cluster.
PS    Tau    In the region of the Pleiades cluster.
PT    Tau    The member of the Pleiades cluster.
PU    Tau    In the region of the Pleiades cluster.
PV    Tau    In the region of the Pleiades cluster. Possible member
PV    Tau    of the cluster.
PW    Tau    In the region of the Pleiades cluster.
PZ    Tau    In the region of the Pleiades cluster.
QQ    Tau    SB2. The member of the Pleiades cluster.
QR    Tau    In the region of the Pleiades cluster.
QS    Tau    In the region of the Pleiades cluster.
QT    Tau    In the region of the Pleiades cluster.
QU    Tau    VB A (B 18.0m, 4.0", 135deg). In the region of the
QU    Tau    Pleiades cluster.
QV    Tau    In the region of the Pleiades cluster.
QW    Tau    In the region of the Pleiades cluster.
QX    Tau    The member of the Pleiades cluster.
QX    Tau    Max = 2444896.79 + 0.483d*E, M - m = 0.5P, A(V) = 0.125m
QX    Tau    [10052].
QY    Tau    In the region of the Pleiades cluster. Not a member
QY    Tau    of the cluster.
QZ    Tau    In the region of the Pleiades cluster.
V0335 Tau    In the region of the Pleiades cluster.
V0336 Tau    In the region of the Pleiades cluster. Possible member
V0336 Tau    of the cluster.
V0337 Tau    In the region of the Pleiades cluster.
V0338 Tau    In the region of the Pleiades cluster. Possible member
V0338 Tau    of the cluster.
V0339 Tau    In the region of the Pleiades cluster. Not a member
V0339 Tau    of the cluster.
V0340 Tau    In the region of the Pleiades cluster.
V0341 Tau    In the region of the Pleiades cluster.
V0342 Tau    In the region of the Pleiades cluster.
V0343 Tau    The member of the Pleiades cluster.
V0344 Tau    In the region of the Pleiades cluster.
V0345 Tau    In the region of the Pleiades cluster.
V0346 Tau    The member of the Pleiades cluster.
V0347 Tau    In the region of the Pleiades cluster. Not a member
V0347 Tau    of the cluster.
V0348 Tau    In the region of the Pleiades cluster.
V0349 Tau    In the region of the Pleiades cluster. Possible member
V0349 Tau    of the cluster.
V0350 Tau    In the region of the Pleiades cluster. Possible member
V0350 Tau    of the cluster.
V0351 Tau    In the region of the Pleiades cluster. Not a member
V0351 Tau    of the cluster.
V0352 Tau    In the region of the Pleiades cluster.
V0353 Tau    In the region of the Pleiades cluster. Possible member
V0353 Tau    of the cluster.
V0354 Tau    In the region of the Pleiades cluster. Possible member
V0354 Tau    of the cluster.
V0355 Tau    In the region of the Pleiades cluster. Possible member
V0355 Tau    of the cluster.
V0356 Tau    In the region of the Pleiades cluster.
V0357 Tau    The member of the Pleiades cluster.
V0358 Tau    The member of the Pleiades cluster.
V0359 Tau    In the region of the Pleiades cluster.
V0360 Tau    In the region of the Pleiades cluster.
V0361 Tau    In the region of the Pleiades cluster. Possible member
V0361 Tau    of the cluster.
V0362 Tau    In the region of the Pleiades cluster.
V0363 Tau    In the region of the Pleiades cluster. Possible member
V0364 Tau    In the region of the Pleiades cluster. Possible member
V0364 Tau    of the cluster.
V0365 Tau    In the region of the Pleiades cluster.
V0366 Tau    The member of the Pleiades cluster.
V0367 Tau    In the region of the Pleiades cluster.
V0368 Tau    In the region of the Pleiades cluster.
V0369 Tau    In the region of the Pleiades cluster.
V0370 Tau    The member of the Pleiades cluster.
V0371 Tau    VB (Delta(m) ~1m, 1.5"). The member of the Pleiades
V0371 Tau    cluster.
V0372 Tau    The member of the Pleiades cluster.
V0373 Tau    In the region of the Pleiades cluster.
V0374 Tau    In the region of the Pleiades cluster.
V0375 Tau    In the region of the Pleiades cluster. Not a member
V0375 Tau    of the cluster.
V0376 Tau    The member of the Pleiades cluster.
V0377 Tau    The member of the Pleiades cluster.
V0378 Tau    The member of the Pleiades cluster.
V0379 Tau    In the region of the Pleiades cluster. Possible member
V0379 Tau    of the cluster.
V0380 Tau    In the region of the Pleiades cluster. Possible member
V0380 Tau    of the cluster.
V0381 Tau    The member of the Pleiades cluster.
V0382 Tau    The member of the Pleiades cluster.
V0383 Tau    In the region of the Pleiades cluster.
V0384 Tau    The member of the Pleiades cluster.
V0385 Tau    In the region of the Pleiades cluster. Not a member
V0385 Tau    of the cluster.
V0386 Tau    TCSN 437. In the region of the Pleiades cluster.
V0387 Tau    In the region of the Pleiades cluster.
V0388 Tau    In the region of the Pleiades cluster.
V0389 Tau    TCSN 439. In the region of the Pleiades cluster.
V0390 Tau    In the region of the Pleiades cluster.
V0392 Tau    In the region of the Pleiades cluster. Possible member
V0392 Tau    of the cluster.
V0394 Tau    In the region of the Pleiades cluster. Not a member
V0394 Tau    of the cluster.
V0395 Tau    In the region of the Pleiades cluster.
V0396 Tau    In the region of the Pleiades cluster.
V0397 Tau    In the region of the Pleiades cluster.
V0398 Tau    In the region of the Pleiades cluster. Possible member
V0398 Tau    of the cluster.
V0399 Tau    The member of the Pleiades cluster.
V0400 Tau    In the region of the Pleiades cluster.
V0401 Tau    In the region of the Pleiades cluster.
V0402 Tau    The member of the Pleiades cluster.
V0403 Tau    The member of the Pleiades cluster.
V0404 Tau    In the region of the Pleiades cluster.
V0405 Tau    In the region of the Pleiades cluster.
V0410 Tau    There are periodical light variations with P = 1.92d,
V0410 Tau    A(V) = 0.21m, M - m = 0.5P [10056].
V0411 Tau    mu = 0.13", P = 143deg.
V0411 Tau    Eruptive white dwarf. Usually there are quasi-perio-
V0411 Tau    dic variations with A ~0.3m and periods P0 = 12.436
V0411 Tau    Min and P1 = 8.237 Min (P1/P0 = 0.6624) which are
V0411 Tau    nonlinearly modulated by the third period PL ~0.135d
V0411 Tau    (probably by the orbital period of a faint companion).
V0421 Tau    Minor planet (586) Thekla.
V0423 Tau    Min II 15.8.
V0425 Tau    In the region of the Pleiades cluster. Not a member
V0425 Tau    of the cluster.
V0426 Tau    In the region of the Pleiades cluster.
V0427 Tau    In the region of the Pleiades cluster.
V0428 Tau    In the region of the Pleiades cluster.
V0429 Tau    In the region of the Pleiades cluster.
V0430 Tau    In the region of the Pleiades cluster. Possible member
V0430 Tau    of the cluster.
V0431 Tau    In the region of the Pleiades cluster.
V0432 Tau    In the region of the Pleiades cluster.
V0433 Tau    In the region of the Pleiades cluster.
V0434 Tau    In the region of the Pleiades cluster.
V0435 Tau    In the region of the Pleiades cluster. Possible member
V0435 Tau    of the cluster.
V0436 Tau    In the region of the Pleiades cluster. Not a member
V0436 Tau    of the cluster.
V0437 Tau    In the region of the Pleiades cluster. Not a member
V0437 Tau    of the cluster.
V0438 Tau    In the region of the Pleiades cluster. Possible member
V0438 Tau    of the cluster.
V0439 Tau    In the region of the Pleiades cluster.
V0440 Tau    In the region of the Pleiades cluster.
V0441 Tau    In the region of the Pleiades cluster. Possible member
V0441 Tau    of the cluster.
V0442 Tau    In the region of the Pleiades cluster.
V0443 Tau    In the region of the Pleiades cluster.
V0444 Tau    In the region of the Pleiades cluster. Possible member
V0444 Tau    of the cluster.
V0445 Tau    In the region of the Pleiades cluster.
V0446 Tau    The member of the Pleiades cluster.
V0447 Tau    In the region of the Pleiades cluster. Not a member
V0447 Tau    of the cluster.
V0448 Tau    The member of the Pleiades cluster.
V0449 Tau    In the region of the Pleiades cluster. Not a member
V0449 Tau    of the cluster.
V0451 Tau    In the region of the Pleiades cluster. Not a member
V0451 Tau    of the cluster.
V0452 Tau    In the region of the Pleiades cluster. Possible member
V0452 Tau    of the cluster.
V0453 Tau    In the region of the Pleiades cluster. Possible member
V0453 Tau    of the cluster.
V0454 Tau    In the region of the Pleiades cluster. Not a member
V0454 Tau    of the cluster.
V0455 Tau    In the region of the Pleiades cluster.
V0456 Tau    In the region of the Pleiades cluster.
V0457 Tau    In the region of the Pleiades cluster.
V0458 Tau    In the region of the Pleiades cluster.
V0459 Tau    In the region of the Pleiades cluster.
V0460 Tau    In the region of the Pleiades cluster.
V0461 Tau    In the region of the Pleiades cluster. Possible member
V0461 Tau    of the cluster.
V0462 Tau    In the region of the Pleiades cluster. Not a member
V0462 Tau    of the cluster.
V0463 Tau    In the region of the Pleiades cluster.
V0464 Tau    In the region of the Pleiades cluster.
V0465 Tau    In the region of the Pleiades cluster.
V0466 Tau    In the region of the Pleiades cluster. Possible member
V0466 Tau    of the cluster.
V0467 Tau    In the region of the Pleiades cluster.
V0468 Tau    In the region of the Pleiades cluster.
V0469 Tau    In the region of the Pleiades cluster.
V0470 Tau    In the region of the Pleiades cluster. Possible member
V0470 Tau    of the cluster.
V0471 Tau    The member of the Hyades cluster. mu alpha =  + 0.117",
V0471 Tau    mu delta = -0.020".
V0471 Tau    EA/D/(RS + WD) + XP. d = 0.0625P.
V0471 Tau    There occurs a total eclipse of the white dwarf in
V0471 Tau    Min I (A = 0.04m V, 0.36m U).
V0471 Tau    P var. Min I = 2440612.67083 + 0.52118321d*E
V0471 Tau    (JD2440570 - 970) [06250]; Min I = 2440898.80038 +
V0471 Tau    0.52118376d*E (JD2440880 - 41360), Min I =
V0471 Tau    2441665.46153 + 0.52118329d*E (JD2441660 -
V0471 Tau    42100) [10058]; since JD2441900 - see Table.
V0471 Tau    Wave-like distorsion with the amplitude from 0.05m
V0471 Tau    up to 0.27m and with the period close to the orbital
V0471 Tau    one is observed in the light curve outside eclipses;
V0471 Tau    sometimes there are also flares. The wave is migrating on
V0471 Tau    phase in the direction of phase decreasing
V0471 Tau    with a migration period of 191d [10060] or ~250d
V0471 Tau    [10061]. The period of white dwarf rotation derived
V0471 Tau    through X-ray observations Ppuls = 554.73s [10062].
V0472 Tau    In the region of the Pleiades cluster.
V0473 Tau    P = 2.7800d?
V0474 Tau    In the region of the Pleiades cluster. Not a member
V0474 Tau    of the cluster.
V0475 Tau    In the region of the Pleiades cluster.
V0476 Tau    In the region of the Pleiades cluster.
V0477 Tau    In the region of the Pleiades cluster.
V0478 Tau    In the region of the Pleiades cluster.
V0479 Tau    VB A (BC 8.90m, 59", 357deg); (k - b)2 = 0.40.
V0480 Tau    VB A (B 10.4m, 176", 303deg). The member of the Hyades
V0480 Tau    cluster.
V0481 Tau    In the region of the Pleiades cluster.
V0483 Tau    The member of the Hyades cluster.
V0484 Tau    The member of the Hyades cluster.
V0485 Tau    In the region of the Pleiades cluster.
V0486 Tau    Epoch of Max (U) is given.
V0486 Tau    P =/ 10.61d? [10063].
V0487 Tau    In the region of the Pleiades cluster. Not a member
V0487 Tau    of the cluster.
V0487 Tau    On the photograph west is at the top and
V0487 Tau    south to the right.
V0488 Tau    The member of the Pleiades cluster.
V0489 Tau    In the region of the Pleiades cluster.
V0490 Tau    In the region of the Pleiades cluster.
V0491 Tau    In the region of the Pleiades cluster. Possible member
V0491 Tau    of the cluster.
V0492 Tau    In the region of the Pleiades cluster. Possible member
V0492 Tau    of the cluster.
V0493 Tau    In the region of the Pleiades cluster.
V0494 Tau    In the region of the Pleiades cluster. Not a member
V0494 Tau    of the cluster.
V0495 Tau    In the region of the Pleiades cluster.
V0496 Tau    In the region of the Pleiades cluster.
V0497 Tau    In the region of the Pleiades cluster. Possible member
V0497 Tau    of the cluster.
V0498 Tau    In the region of the Pleiades cluster. Not a member
V0498 Tau    of the cluster.
V0499 Tau    In the region of the Pleiades cluster.
V0500 Tau    The member of the Pleiades cluster.
V0501 Tau    In the region of the Pleiades cluster. Not a member
V0501 Tau    of the cluster.
V0502 Tau    The member of the Pleiades cluster.
V0503 Tau    In the region of the Pleiades cluster. Not a member
V0503 Tau    of the cluster.
V0504 Tau    In the region of the Pleiades cluster.
V0506 Tau    In the region of the Pleiades cluster. Not a member
V0506 Tau    of the cluster.
V0507 Tau    In the region of the Pleiades cluster.
V0508 Tau    In the region of the Pleiades cluster.
V0509 Tau    In the region of the Pleiades cluster.
V0510 Tau    In the region of the Pleiades cluster.
V0511 Tau    In the region of the Pleiades cluster.
V0512 Tau    In the region of the Pleiades cluster.
V0513 Tau    In the region of the Pleiades cluster.
V0514 Tau    In the region of the Pleiades cluster.
V0515 Tau    In the region of the Pleiades cluster.
V0516 Tau    In the region of the Pleiades cluster.
V0517 Tau    In the region of the Pleiades cluster. Not a member
V0517 Tau    of the cluster.
V0518 Tau    VB B (A 14.4m; B 10", 80deg). The member of the
V0518 Tau    Pleiades cluster.
V0519 Tau    In the region of the Pleiades cluster. Not a member
V0519 Tau    of the cluster.
V0520 Tau    In the region of the Pleiades cluster. Possible member
V0520 Tau    of the cluster.
V0521 Tau    In the region of the Pleiades cluster. Not a member
V0521 Tau    of the cluster.
V0522 Tau    In the region of the Pleiades cluster.
V0523 Tau    In the region of the Pleiades cluster. Not a member
V0523 Tau    of the cluster.
V0524 Tau    In the region of the Pleiades cluster.
V0525 Tau    In the region of the Pleiades cluster. Not a member
V0525 Tau    of the cluster.
V0526 Tau    In the region of the Pleiades cluster.
V0527 Tau    In the region of the Pleiades cluster. Not a member
V0527 Tau    of the cluster.
V0528 Tau    In the region of the Pleiades cluster.
V0529 Tau    In the region of the Pleiades cluster. Not a member
V0529 Tau    of the cluster.
V0530 Tau    In the region of the Pleiades cluster. Not a member
V0530 Tau    of the cluster.
V0531 Tau    In the region of the Pleiades cluster.
V0532 Tau    In the region of the Pleiades cluster.
V0533 Tau    In the region of the Pleiades cluster.
V0534 Tau    In the region of the Pleiades cluster.
V0535 Tau    In the region of the Pleiades cluster.
V0536 Tau    In the region of the Pleiades cluster.
V0537 Tau    In the region of the Pleiades cluster.
V0538 Tau    The member of the Pleiadea cluster.
V0539 Tau    In the region of the Pleiades cluster. Possible member
V0539 Tau    of the cluster.
V0540 Tau    The member of the Pleiades cluster.
V0541 Tau    The member of the Pleiades cluster.
V0542 Tau    In the region of the Pleiades cluster. Not a member
V0542 Tau    of the cluster.
V0543 Tau    In the region of the Pleiades cluster.
V0544 Tau    In the region of the Pleiades cluster.
V0545 Tau    Max = 2444896.678 + 0.355d*E, M - m = 0.42P, A(V) =
V0545 Tau    0.09m [10052]. The member of the Pleiades cluster.
V0546 Tau    In the region of the Pleiades cluster. Not a member
V0546 Tau    of the cluster.
V0547 Tau    In the region of the Pleiades cluster.
V0548 Tau    In the region of the Pleiades cluster. Possible member
V0548 Tau    of the cluster.
V0549 Tau    In the region of the Pleiades cluster.
V0550 Tau    The member of the Pleiades cluster.
V0551 Tau    In the region of the Pleiades cluster.
V0552 Tau    In the region of the Pleiades cluster.
V0553 Tau    In the region of the Pleiades cluster. Not a member
V0553 Tau    of the cluster.
V0554 Tau    In the region of the Pleiades cluster.
V0555 Tau    In the region of the Pleiades cluster. Not a member
V0555 Tau    of the cluster.
V0556 Tau    In the region of the Pleiades cluster.
V0557 Tau    In the region of the Pleiades cluster. Not a member
V0557 Tau    of the cluster.
V0558 Tau    In the region of the Pleiades cluster.
V0559 Tau    In the region of the Pleiades cluster. Not a member
V0559 Tau    of the cluster.
V0560 Tau    In the region of the Pleiades cluster. Not a member
V0560 Tau    of the cluster.
V0561 Tau    In the region of the Pleiades cluster.
V0562 Tau    In the region of the Pleiades cluster.
V0563 Tau    In the region of the Pleiades cluster.
V0564 Tau    In the region of the Pleiades cluster.
V0565 Tau    In the region of the Pleiades cluster. Not a member
V0565 Tau    of the cluster.
V0566 Tau    In the region of the Pleiades cluster. Not a member
V0566 Tau    of the cluster.
V0567 Tau    In the region of the Pleiades cluster.
V0568 Tau    In the region of the Pleiades cluster.
V0569 Tau    In the region of the Pleiades cluster. Not a member
V0569 Tau    of the cluster.
V0570 Tau    In the region of the Pleiades cluster.
V0571 Tau    In the region of the Pleiades cluster.
V0572 Tau    In the region of the Pleiades cluster.
V0573 Tau    In the region of the Pleiades cluster.
V0574 Tau    In the region of the Pleiades cluster.
V0575 Tau    In the region of the Pleiades cluster.
V0576 Tau    In the region of the Pleiades cluster.
V0577 Tau    In the region of the Pleiades cluster.
V0578 Tau    In the region of the Pleiades cluster. Not a member
V0578 Tau    of the cluster.
V0579 Tau    In the region of the Pleiades cluster.
V0581 Tau    In the region of the Pleiades cluster.
V0582 Tau    In the region of the Pleiades cluster.
V0583 Tau    In the region of the Pleiades cluster.
V0584 Tau    In the region of the Pleiades cluster.
V0585 Tau    In the region of the Hyades cluster.
V0589 Tau    In the region of the Hyades cluster.
V0594 Tau    In the region of the Pleiades cluster.
V0595 Tau    In the region of the Pleiades cluster.
V0596 Tau    In the region of the Pleiades cluster. Possible member
V0596 Tau    of the cluster.
V0597 Tau    In the region of the Pleiades cluster.
V0598 Tau    In the region of the Pleiades cluster.
V0599 Tau    In the region of the Pleiades cluster.
V0600 Tau    In the region of the Pleiades cluster.
V0601 Tau    In the region of the Pleiades cluster.
V0602 Tau    In the region of the Pleiades cluster. Not a member
V0602 Tau    of the cluster.
V0603 Tau    In the region of the Pleiades cluster.
V0604 Tau    In the region of the Pleiades cluster.
V0605 Tau    In the region of the Pleiades cluster.
V0606 Tau    In the region of the Pleiades cluster.
V0607 Tau    In the region of the Pleiades cluster.
V0608 Tau    In the region of the Pleiades cluster. Not a member
V0608 Tau    of the cluster.
V0609 Tau    In the region of the Pleiades cluster.
V0610 Tau    The member of the Pleiades cluster.
V0611 Tau    In the region of the Pleiades cluster.
V0612 Tau    In the region of the Pleiades cluster.
V0613 Tau    In the region of the Pleiades cluster. Possible member
V0613 Tau    of the cluster.
V0614 Tau    In the region of the Pleiades cluster.
V0615 Tau    In the region of the Pleiades cluster. Not a member
V0615 Tau    of the cluster.
V0617 Tau    In the region of the Pleiades cluster.
V0618 Tau    In the region of the Pleiades cluster.
V0619 Tau    In the region of the Pleiades cluster.
V0620 Tau    In the region of the Pleiades cluster.
V0621 Tau    In the region of the Pleiades cluster.
V0622 Tau    In the region of the Pleiades cluster.
V0623 Tau    The member of the Pleiades cluster.
V0624 Tau    The value of P1(A1 = 0.01m) is given in the Table.
V0624 Tau    P2 = 0.017d, A2 = 0.007m. The member of the Pleiades
V0624 Tau    cluster.
V0625 Tau    In the region of the Pleiades cluster.
V0626 Tau    In the region of the Pleiades cluster.
V0627 Tau    The member of the Pleiades cluster.
V0629 Tau    In the region of the Pleiades cluster.
V0630 Tau    In the region of the Pleiades cluster.
V0631 Tau    The member of the Pleiades cluster.
V0632 Tau    The member of the Pleiades cluster.
V0633 Tau    In the region of the Pleiades cluster. Not a member
V0633 Tau    of the cluster.
V0634 Tau    In the region of the Pleiades cluster. Not a member
V0634 Tau    of the cluster.
V0635 Tau    The member of the Pleiades cluster.
V0636 Tau    In the region of the Pleiades cluster. Not a member
V0636 Tau    of the cluster.
V0637 Tau    In the region of the Pleiades cluster.
V0638 Tau    The member of the Pleiades cluster.
V0639 Tau    In the region of the Pleiades cluster.
V0640 Tau    In the region of the Pleiades cluster.
V0641 Tau    Max = 2444896.744 + 1.22d*E; M - m = 0.5P, A(V) = 0.03m
V0641 Tau    [10052]. The member of the Pleiades cluster.
V0642 Tau    The member of the Pleiades cluster.
V0643 Tau    The member of the Pleiades cluster.
V0644 Tau    The member of the Pleiades cluster.
V0645 Tau    In the region of the Pleiades cluster. Possible member
V0645 Tau    of the cluster.
V0646 Tau    The member of the Pleiades cluster.
V0647 Tau    The value
V0647 Tau    of P1(A1 = 0.011m) is given in the Table.
V0647 Tau    P2 = 0.070d, A2 = 0.006m. The member of the Pleiades
V0647 Tau    cluster.
V0648 Tau    In the region of the Pleiades cluster.
V0649 Tau    In the region of the Pleiades cluster.
V0650 Tau    The member of the Pleiades cluster.
V0651 Tau    In the region of the Pleiades cluster.
V0652 Tau    The member of the Pleiades cluster.
V0653 Tau    In the region of the Pleiades cluster. Not a member
V0653 Tau    of the cluster.
V0654 Tau    In the region of the Pleiades cluster. Possible member
V0654 Tau    of the cluster.
V0655 Tau    In the region of the Pleiades cluster.
V0656 Tau    In the region of the Pleiades cluster.
V0657 Tau    In the region of the Pleiades cluster. Not a member
V0657 Tau    of the cluster.
V0658 Tau    In the region of the Pleiades cluster.
V0659 Tau    In the region of the Pleiades cluster.
V0660 Tau    Max = 2444896.453 + 0.23541d*E, M - m = 0.5P, A(V) =
V0660 Tau    0.20m [10052]. The member of the Pleiades cluster.
V0661 Tau    In the region of the Pleiades cluster.
V0662 Tau    In the region of the Pleiades cluster.
V0663 Tau    In the region of the Pleiades cluster.
V0664 Tau    The member of the Pleiades cluster.
V0665 Tau    In the region of the Pleiades cluster. Not a member
V0665 Tau    of the region.
V0666 Tau    In the region of the Pleiades cluster.
V0667 Tau    The member of the Pleiades cluster.
V0668 Tau    In the region of the Pleiades cluster.
V0669 Tau    In the region of the Pleiades cluster.
V0670 Tau    In the region of the Pleiades cluster.
V0671 Tau    In the region of the Pleiades cluster.
V0672 Tau    In the region of the Pleiades cluster. Not a member
V0672 Tau    of the cluster.
V0673 Tau    In the region of the Pleiades cluster. Possible member
V0673 Tau    of the cluster.
V0674 Tau    In the region of the Pleiades cluster.
V0675 Tau    In the region of the Pleiades cluster. Not a member
V0675 Tau    of the cluster.
V0676 Tau    In the region of the Pleiades cluster.
V0677 Tau    The member of the Pleiades cluster.
V0678 Tau    In the region of the Pleiades cluster. Not a member
V0678 Tau    of the cluster.
V0679 Tau    The member of the Pleiades cluster.
V0680 Tau    In the region of the Pleiades cluster. Not a member
V0680 Tau    of the cluster.
V0681 Tau    In the region of the Pleiades cluster.
V0682 Tau    In the region of the Pleiades cluster.
V0683 Tau    In the region of the Pleiades cluster.
V0684 Tau    In the region of the Pleiades cluster. Not a member
V0684 Tau    of the cluster.
V0685 Tau    In the region of the Pleiades cluster. Not a member
V0685 Tau    of the cluster.
V0686 Tau    In the region of the Pleiades cluster.
V0687 Tau    In the region of the Pleiades cluster.
V0688 Tau    In the region of the Pleiades cluster.
V0689 Tau    In the region of the Pleiades cluster.
V0690 Tau    In the region of the Pleiades cluster.
V0691 Tau    In the region of the Pleiades cluster.
V0692 Tau    In the region of the Pleiades cluster. Possible member
V0692 Tau    of the cluster.
V0693 Tau    In the region of the Pleiades cluster.
V0694 Tau    In the region of the Pleiades cluster.
V0696 Tau    The member of the Hyades cluster.
V0697 Tau    The member of the Hyades cluster.
V0698 Tau    Type INB?
V0700 Tau    The member of the Pleiades cluster.
V0701 Tau    In the region of the Pleiades cluster.
V0702 Tau    In the region of the Pleiades cluster.
V0703 Tau    The member of the Pleiades cluster.
V0705 Tau    In the region of the Pleiades cluster.
V0706 Tau    In the region of the Pleiades cluster.
V0707 Tau    In the region of the Pleiades cluster.
V0709 Tau    In the region of the Pleiades cluster.
V0710 Tau    VB A (B 16m, 3.5", 180deg).
V0711 Tau    VB A (B 8.83m, A = 8.023", E = 0.18, Porb = 2101 yr);
V0711 Tau    SB2 (Porb = 2.83774d [10070]).
V0711 Tau    Migration period of the distortion wave is about
V0711 Tau    10.5 yr [10072].
V0711 Tau    The range of combined light variation is given.
V0712 Tau    In the region of the Pleiades cluster.
V0713 Tau    In the region of the Pleiades cluster.
V0714 Tau    In the region of the Pleiades cluster.
V0715 Tau    In the region of the Pleiades cluster.
V0716 Tau    In the region of the Pleiades cluster.
V0717 Tau    In the region of the Pleiades cluster.
V0718 Tau    In the region of the Hyades cluster.
V0725 Tau    SB1 (Porb = 110.8d [10076]).
V0725 Tau    X-ray outbursts occur periodically near
V0725 Tau    the periastron passages of the pulsar with P = Porb.
V0725 Tau    The amplitude of the corresponding variations of
V0725 Tau    visual brightness of the system A(V) = 0.03m. The period
V0725 Tau    of pulsar rotation Prot var [10077].
V0725 Tau    Prot = 104.17s (JD2442531), 103.806s (JD2442728),
V0725 Tau    103.882s (JD2443505), 103.8402s (JD2443620)
V0725 Tau    [10074]; 103.647s (JD2444521), 103.423s
V0725 Tau    (JD2445292), 103.3429ss(JD2445623) [10078].
V0726 Tau    Min II 11.2.
V0727 Tau    In the region of the Pleiades cluster.
V0728 Tau    In the region of the Pleiades cluster. Not a member
V0728 Tau    of the cluster.
V0729 Tau    Max = 2439024.46 + 152.35d*E (JD2438680 - 39415);
V0729 Tau    Max = 2440127.78 + 313.86d*E (JD2439415 - 40510).
V0729 Tau    H2O maser.
V0732 Tau    In the region of the Pleiades cluster.
V0733 Tau    In the region of the Pleiades cluster.
V0734 Tau    In the region of the Pleiades cluster.
V0735 Tau    In the region of the Pleiades cluster.
V0736 Tau    In the region of the Pleiades cluster.
V0737 Tau    In the region of the Pleiades cluster.
V0738 Tau    In the region of the Pleiades cluster. The chart in [08559]
V0738 Tau    is wrong.
V0739 Tau    In the region of the Pleiades cluster.
V0740 Tau    In the region of the Pleiades cluster.
V0741 Tau    In the region of the Pleiades cluster.
V0742 Tau    In the region of the Pleiades cluster.
V0743 Tau    In the region of the Pleiades cluster.
V0744 Tau    In the region of the Pleiades cluster.
V0746 Tau    In the region of the Pleiades cluster.
V0747 Tau    In the region of the Pleiades cluster.
V0748 Tau    In the region of the Pleiades cluster.
V0749 Tau    In the region of the Pleiades cluster.
V0750 Tau    In the region of the Pleiades cluster.
V0751 Tau    In the region of the Pleiades cluster.
V0752 Tau    In the region of the Pleiades cluster.
V0753 Tau    In the region of the Pleiades cluster. Not a member
V0753 Tau    of the cluster.
V0754 Tau    In the region of the Pleiades cluster.
V0755 Tau    In the region of the Pleiades cluster.
V0756 Tau    In the region of the Pleiades cluster.
V0757 Tau    In the region of the Pleiades cluster.
V0758 Tau    In the region of the Pleiades cluster. Not a member
V0758 Tau    of the cluster.
V0759 Tau    In the region of the Pleiades cluster.
V0760 Tau    In the region of the Pleiades cluster.
V0761 Tau    In the region of the Pleiades cluster. Not a member
V0761 Tau    of the cluster.
V0762 Tau    In the region of the Pleiades cluster. Not a member
V0762 Tau    of the cluster.
V0763 Tau    In the region of the Pleiades cluster.
V0764 Tau    In the region of the Pleiades cluster.
V0765 Tau    In the region of the Pleiades cluster.
V0767 Tau    In the region of the Pleiades cluster.
V0768 Tau    In the region of the Pleiades cluster.
V0769 Tau    In the region of the Pleiades cluster.
V0770 Tau    In the region of the Pleiades cluster.
V0771 Tau    In the region of the Pleiades cluster.
V0772 Tau    In the region of the Pleiades cluster.
V0773 Tau    There are also quasisinusoidal light variations with
V0773 Tau    P = 3.43d and A(V) = 0.13m [10056].
V0774 Tau    VB A (B 6.96m, G5IV, 66.8", 315deg).
V0775 Tau    The member of the Hyades cluster.
V0776 Tau    VB A (B 7.5m, 1.4", 333deg, 1958; C 8.7m, 77.2", 233deg,
V0776 Tau    1925); SB1 (Porb = 57.25d). The member of the
V0776 Tau    Hyades cluster.
V0777 Tau    VB A (B 8.12m V, 0.0088", 173.2deg, 1980.6).
V0777 Tau    The member of the Hyades cluster.
V0778 Tau    Min II 17.0. P var. Min I = 2438680.546 + 0.434842d*E
V0778 Tau    (JD2436528 - 38841); Min I = 2439765.488 + 0.434846d*E
V0778 Tau    (JD2439559 - 41031); since JD2440129 - see Table.
V0780 Tau    VB A (B 15.8m V, 0.3", 310deg, 1974); mu = 0.364",
V0780 Tau    P = 163deg.
V0781 Tau    Min II 9.3.
V0782 Tau    In the region of the Pleiades cluster.
V0783 Tau    In the region of the Pleiades cluster.
V0784 Tau    In the region of the Pleiades cluster.
V0785 Tau    The member of the Pleiades cluster.
V0787 Tau    In the region of the Pleiades cluster.
V0788 Tau    In the region of the Pleiades cluster.
V0789 Tau    The member of the Pleiades cluster.
V0790 Tau    The member of the Pleiades cluster.
V0791 Tau    In the region of the Pleiades cluster.
V0792 Tau    Near V752 Tau. Identical to it?
V0792 Tau    In the region of the Pleiades cluster.
V0793 Tau    The member of the Pleiades cluster.
V0794 Tau    In the region of the Pleiades cluster. Not a member
V0794 Tau    of the cluster.
V0795 Tau    In the region of the Pleiades cluster.
V0796 Tau    The member of the Pleiades cluster.
V0797 Tau    In the region of the Pleiades cluster. Not a member
V0797 Tau    of the cluster.
V0798 Tau    In the region of the Pleiades cluster.
V0799 Tau    In the region of the Pleiades cluster.
V0800 Tau    In the region of the Pleiades cluster.
V0801 Tau    In the region of the Pleiades cluster.
V0802 Tau    In the region of the Pleiades cluster.
V0804 Tau    In the region of the Pleiades cluster.
V0805 Tau    The member of the Hyades cluster.
V0807 Tau    VB A (B = GH Tau, 21.4", 193deg).
V0808 Tau    Porb = 11.93d. The member of the Hyades cluster.
V1144 Tau    SB, Porb = 13.88d.
V1148 Tau    Type LBV: is also possible. SB, Porb = 2.2075d.
V1152 Tau    Type E: with P = 11.080d is also possible.
V1161 Tau    Variability needs confirmation.
V1212 Tau    Dwarf nova in Taurus.
V1226 Tau    Variable brown dwarf.
V1229 Tau    MinII 6.88.
V1230 Tau    MinII 14.49.
V1234 Tau    MinII 12.9.
V1237 Tau    The depth of MinII is 0.19.
V1238 Tau    MinII 8.87.
V1239 Tau    MinII 10.76.
V1241 Tau    The depth of Min II 0.22m. The primary component var,
V1241 Tau    DSCT:,  P1 = 0.16454d, P2 = 0.13721d.
V1243 Tau    VB (A 9.1m var, F1; B 9.9m, F8:, 0.3", 24deg, 1991).
V1248 Tau    OH maser.
V1258 Tau    SiO maser.
V1260 Tau    MinII - MinI = 0.57P.
V1268 Tau    VB A (B 7.8m, A2V, 7", 207deg, 2004).
V1282 Tau    SB2, Porb > 6000d?
V1283 Tau    SB1, Porb = 7.05051d.
V1284 Tau    Min II = 15.17.
V1287 Tau    Min II = < 8.69. MinII - MinI = 0.39P.
V1295 Tau    Min II = 11.35.
V1299 Tau    VB AB (9.3m, 9.3m, 0".4, 252deg, 2007).
V1304 Tau    SB.
V1305 Tau    Amplitude(Min II)=  0.2mag.
V1311 Tau    Min II = 14.59.
V1322 Tau    P = 0.585d is also possible.
V1326 Tau    P = 1.651d is also possible.
V1332 Tau    Min II = 11.78. Possily a pulsating star with a twice shorter period.
V1337 Tau    SB2.
V1345 Tau    P = 11.66d is also effect.
V1347 Tau    SB2.
V1350 Tau    SB2.
V1352 Tau    Min II = 13.1 :.
V1355 Tau    Min II = 14.2.
V1356 Tau    Min II = 11.37. MinII - MinI = 0.57P.
V1364 Tau    VB AB.
V1367 Tau    Min II = 11.15.
V1369 Tau    Min II = 12.43.
V1370 Tau    Min II = 11.28.
V1374 Tau    Min II = 13.9.
alf   Tau    VB A (B 13.5m, M2V, 31", 110deg).
alf   Tau    The star is surrounded by an infrared emission envelope
alf   Tau    with the diameter of about 10". In the region of the
alf   Tau    Hyades cluster.
zet   Tau    Min II 3.05.
tet 2 Tau    VB A (B 4.85m, 0.02077", 19.6deg, 1980.59); SB1 (Porb =
tet 2 Tau    140.728D, E = 0.75 [10087]). The value of P1(A1 = 0.017m B)
tet 2 Tau    is given in the Table. P1 var. Later P1 = 0.07541d
tet 2 Tau    (A1 = 0.023m B), P2 = 0.0831d (A2 = 0.013m B). Possibly
tet 2 Tau    eclipsing with the elements:
tet 2 Tau    Min = 2445358.38 + 140.734d*E, A = 0.02m B.
tet 2 Tau    The member of the Hyades cluster.
lam   Tau    Min II 3.54. Triple system. The eclipsing system rotates
lam   Tau    around the third component with P = 33.025d [10090].
lam   Tau    In the region of the Hyades cluster.
rho   Tau    The member of the Hyades cluster.
ups   Tau    VB A (B 6.5m, 0.020"). The member of the Hyades cluster.
S     Tel    The AAVSO chart, approved by Harvard Observatory in 1951,
S     Tel    corresponds to the star at the coordinates in the Table. Most
S     Tel    observations of S Tel reported in the 20th century probably
S     Tel    refer to this star. There remains doubt if the original
S     Tel    CPD-55 9313 was the same star [00126].
U     Tel    P var [00000]. SiO maser.
RR    Tel    A symbiotic Nova. In 1889 - 1930, 12m - 14m pg (according to
RR    Tel    [00123], irregular variations; according to [00128],
RR    Tel    Max = 2411490 + 384d*E, with irregularities). In 1930 - 1944,
RR    Tel    12.5m - 16.5m pg, Max = 2430145 + 386.73d*E [00125]. An outburst
RR    Tel    from 14m to 7m in October, 1944. On JD2441426 - 2444899,
RR    Tel    5.06m - 6.74m J, P = 387d [00124]. The data in [00002] reveal
RR    Tel    current V-band variations with a small amplitude and nearly
RR    Tel    the same period [00000]. A period of 11.38 years, presumably the
RR    Tel    orbital one, was reported in [00127]. The spectrum in the Max of
RR    Tel    the outburst was F5 without emissions, then a rich emission
RR    Tel    spectrum was formed. Since the 1970s, TiO absorption bands are
RR    Tel    being noted. Radio source, soft X-ray source.
RS    Tel    Semiregular variations, P = 49.0d [00002].
RV    Tel    d = 0.02P. VB (0.6", 294deg, 1946).
SS    Tel    SiO maser.
ST    Tel    The chart in [06286] is wrong.
SU    Tel    VB B (A 13.6m B, 12" nf).
TY    Tel    OH, SiO maser.
UY    Tel    VB.
YY    Tel    No emission lines in the spectrum.
AB    Tel    Min II = 12.9.
AG    Tel    VB A (B 13.7m B, 20" sp).
AN    Tel    A secondary period about 27d.
AV    Tel    Min II = 14.1.
AW    Tel    Min II = 12.3.
AX    Tel    [A/H] = -0.7.
BB    Tel    Not red [00000].
BI    Tel    [Fe/H] = -1.96.
BL    Tel    [Fe/H] = -0.66. The depth of Min II is about 0.1m. The primary
BL    Tel    component varies approximately between 7.09m and 7.27m V,
BL    Tel    the periods revealed in these pulastins are 92.5d and 64.8d
BL    Tel    [00138].
BO    Tel    [A/H] = -0.3.
CK    Tel    VB B (A 15.0m, 12" s).
DZ    Tel    VB A (B 15.9m, 15" np).
EH    Tel    VB A (B 15.6m R, 5" nf).
EU    Tel    The chart in [06286] is wrong.
FL    Tel    Min II = 14.5.
FX    Tel    VB (4").
GM    Tel    VB A (B 16.6m, 10" p).
GY    Tel    Min II = 11.83.
HH    Tel    [Fe/H] = -1.02.
HM    Tel    Min II = 12.3.
HO    Tel    Min II = 8.67.
HR    Tel    Type EW with a twice longer period is possible.
HY    Tel    [Fe/H] = -0.17.
IQ    Tel    Min II = 12.4.
IS    Tel    Min II = 9.82.
IZ    Tel    Min II = 12.2.
KK    Tel    Porb = 0.08453d.
KN    Tel    VB A (B 15.6m B, 13" sf).
LW    Tel    Possibly identical to NSV 10695.
MT    Tel    [Fe/H] = -1.85.
MY    Tel    Min II = 13.5.
NN    Tel    Min II = 15.5.
NP    Tel    Min II = 13.3.
NS    Tel    Min II = 9.8. Strong O'Connell effect.
NV    Tel    Min II = 9.83.
PR    Tel    Min II = 11.4.
PS    Tel    V39 (NGC 6584). Cluster non-member?
PS    Tel    P = 0.1422d or 0.1657d is possible.
PT    Tel    V27 (NGC 6584). Cluster non-member.
PU    Tel    V24 (NGC 6584). Cluster non-member.
PV    Tel    SB2.
PX    Tel    V15 (NGC 6584). Cluster non-member.
QR    Tel    P(osc) = 13.0 min.
QS    Tel    Porb = 0.097187d.
QU    Tel    Multiperiodic, P = 257s is dominant.
QW    Tel    Min II = 7.67.
QY    Tel    Min II = 10.06.
QZ    Tel    Min II = 8.27. VB B (A 9" sp). The variability is probably due to the fainter
QZ    Tel    (B) component [00075]. The variability range for combined light
QZ    Tel    is given.
V0337 Tel    Min II = 10.20.
V0340 Tel    The data from [00002] do not confirm the tabulated period
V0340 Tel    [00000].
V0343 Tel    Min II = 9.40. O'Connell effect, MaxII 9.18m.
V0349 Tel    Multiperiodic, P2 = 1.2719d.
V0351 Tel    Min II = 10.27.
V0356 Tel    MinII - MinI = 0.48P.
V0358 Tel    A twice shorter period is not excluded.
V0359 Tel    MinII - MinI = 0.78P. VB (8.8m, 11.4m, 4", 239deg, 1991).
V0362 Tel    VB (9.5m, 12.2m, 3", 140deg, 1991).
V0374 Tel    The first-overtone period is tabulated; for the fundamental mode, P = 0.47907d.
V0379 Tel    VB A (B 18.52m, 2.4").
V0381 Tel    VB (11", 6deg, 2000); combined magnitudes are tabulated. For the first-overtone period, see the Table; P0 = 0.46781d; the amplitude ratio (1O/F) is 1.05.
R     Tri    P var. Max = 2412167 + 267.3d*E (JD2412000 - 16000);
R     Tri    Max = 2416972 + 262.6d*E (JD2416000 - 20000);
R     Tri    since JD2420000 - see Table. Maser (H2O).
S     Tri    P var. Max = 2418541 + 248.9d*E (JD2418000 - 31000);
S     Tri    since JD2431000 - see Table.
T     Tri    P var. Max = 2420535 + 320.6d*E (JD2420000 - 27000);
T     Tri    since JD2427000 - see Table.
U     Tri    Delta(S) = 1.3.
V     Tri    Min II 11.0.
X     Tri    VB A (B 13.3m, 6.7", 55.3deg, 1952). Usual brightness in
X     Tri    Max 8.88. d = 0.013P; Min II 9.07. According to [10043],
X     Tri    a two-peaked flare-like event of 35 min duration
X     Tri    (Delta(V) = 0.33m) was observed at JD2445594.4550.
X     Tri    P var. Min = 2422722.269 + 0.9715342d*E
X     Tri    (JD2422700 - 26600); Min = 2426946.508 + 0.9715390d*E
X     Tri    (JD2426600 - 33400); Min = 2433504.397 + 0.9715290d*E
X     Tri    (JD2433400 - 35500);
X     Tri    Min = 2435687.422 + 0.9715352d*E (JD2435500 - 39200);
X     Tri    Min = 2439375.373 + 0.9715277d*E
X     Tri    (JD2439200 - 42500) [07603]; since JD2442500 - see Table.
Y     Tri    Var No.2 (M33). VB A (B 17.28m B, 26.4" np).
RS    Tri    VB A (B 11.98m, 6.0", 214deg, 1962).
RS    Tri    d = 0.016P; Min II 10.4, Min II - Min I = 0.56P.
RU    Tri    VB A (B 12m, 21.8", 88deg). Min II 11.8:.
RW    Tri    The depth of Min I 1.12m - 2.21m.
RW    Tri    D = 0.052P - 0.086P, d ~0.03P. P var? [03434, 09858, 9859].
RW    Tri    Strong fluctuations of light outside eclipses. the lower
RW    Tri    the brightness outside the eclipse, the deeper the Min.
RW    Tri    In J, K light Min II of 0.16m J depth was found at the
RW    Tri    phase 0.50P [10053]. Flat spectrum of the accretion disc
RW    Tri    with emission lines.
RX    Tri    Max = 2426577 + 192d*E (JD2426500 - 31800);
RX    Tri    since JD2432800 - see Table. According to [04029],
RX    Tri    P = 100d?
RY    Tri    Red.
ST    Tri    Min II 14.5.
SW    Tri    Blazhko effect is possible.
SY    Tri    Blazhko effect is possible.
TT    Tri    In the region of the galaxy M 33.
TZ    Tri    ADS 1697 A (B 6.72m, F6V, SB2, Porb = 2.2365d,
TZ    Tri    3.9", 71deg, 1973); SB2 (P = 14.732d). Secondary
TZ    Tri    variations on ~100d time scale. H and K CaII emission was
TZ    Tri    noted only for one of the two G-stars.
AW    Tri    Min II = 13.7.
AY    Tri    Min II = 14.45.
AZ    Tri    Min II = 14.3.
BB    Tri    Min II = 14.3 :.
BC    Tri    Min II = 12.08. Type RRC with a twice shorter period is possible.
BE    Tri    Min II = 13.2.
BF    Tri    Min II = 14.5 :.
BI    Tri    Min II = 12.65. VB AB (4", 227deg, 1997).
BM    Tri    Min II = 13.3 :.
BO    Tri    Min II = 12.0.
BP    Tri    Min II = 14.6.
BQ    Tri    Min II = 12.8.
BR    Tri    Min II = 13.3.
BT    Tri    Min II = 14.7.
BU    Tri    Min II = 14.9.
BV    Tri    Min II = 14.3.
BX    Tri    Min II = 12.60.
CC    Tri    Min II = 13.6.
CD    Tri    Min II = 12.3.
CL    Tri    Min II = 12.07.
CM    Tri    Min II = 14.3.
CN    Tri    Min II = 12.25.
CP    Tri    Min II = 10.95. The identification with the missed BD star, BD +33 460 = NSV 00856, suggested in [121] seems unjustified.
CR    Tri    Min II = 14.7.
CS    Tri    Min II = 11.4.
alf   Tri    SB (Porb = 1.767 d).
R     TrA    SB?
U     TrA    For moments of Max0 (fundamental mode) see Table.
U     TrA    Max1 (first overtone) = 2443266.05 + 1.824881d*E.
RR    TrA    Min II 10.60, dII = 0.025P.
RW    TrA    (k - b)2 = 0.30. Delta(S) = 1.
SU    TrA    The chart in [06286] is wrong.
TW    TrA    VB.
TY    TrA    The chart in [06286] is wrong.
UW    TrA    The chart in [06286] is wrong.
UZ    TrA    The chart in [06286] is wrong.
XX    TrA    The chart in [06286] is wrong.
XY    TrA    The chart in [06286] is wrong.
BH    TrA    According to [04637], L type.
CI    TrA    Possibly P < 0.3d.
DI    TrA    The chart in [06286] is wrong.
DV    TrA    Three Max and three Min are observed during a cycle.
DV    TrA    Max1 (phi = 0.0P) 13.2m; Max2 (phi = 0.2P) 14.2m; Max3
DV    TrA    (phi = 0.6P) 13.5m. Min1, Min2, Min3 ~16.0m.
DZ    TrA    The chart in [06286] is wrong.
EH    TrA    Shallow Min II is possible.
EK    TrA    n star of a pair.
EK    TrA    For the mean cycle between normal maxima see Table. The
EK    TrA    mean cycle between supermaxima 442.1d (JD2435200 - 39700),
EK    TrA    551.5d (JD2439700 - 44050). Superhumps (delta(M) = 0.26m V)
EK    TrA    with P = 0.06492d, M - m = 0.26P [09945].
EL    TrA    Min II 10.9.
EM    TrA    Min II 10.4.
EN    TrA    According to [07934], RV: type.
EP    TrA    Min II 9.5.
EQ    TrA    Min II 9.0.
EQ    TrA    P var. Min = 2416267.614 + 2.709220d*E (JD2416000 - 29000);
EQ    TrA    since JD2429000 - see Table.
ER    TrA    P > 220d.
FH    TrA    The elements need confirmation.
FK    TrA    The elements need confirmation.
FM    TrA    P >= 220d.
GN    TrA    Min II 12.0.
HP    TrA    Deep Min II. The elements need improvement.
HV    TrA    Min II? 14.8. Min II - Min I = 0.55P.
IM    TrA    P >= 150d. Epoch of Min is given.
IW    TrA    Min II 14.5:. The elements need confirmation.
KX    TrA    2U 1639-62? P.K.326 -10deg 1. Gas velocities up to
KX    TrA    5000 km/s [09958].
KY    TrA    TrA X-1 = A1524-61.
KZ    TrA    4U 1626-67. Lx/Lopt ~2000. VB B (A 14.9m; B25", 189deg).
KZ    TrA    Barycentric period parameters for pulses [04534]: Min =
KZ    TrA    JED 2443931.2394789; P = 7.6776762s, DP/dt =
KZ    TrA    (-4.95 +-0.02)*10**(-11). Delta(m) pulse = 0.02m - 0.17m.
KZ    TrA    Porb = 2491.06s or 2492.32s [04558].
KZ    TrA    Flares with Delta(m) up to 0.4m with intervals ~20 min
KZ    TrA    correlated with X-ray flares [04536].
LM    TrA    The chart in [08661] is wrong.
LP    TrA    VB A (B 11.5m, 25", 123deg; C 12.0m, BC 6").
MZ    TrA    MinII 8.73.
NO    TrA    MinII 8.85.
NT    TrA    MinII - MinI = 0.57P.
NY    TrA    VB A (B 5", 62deg, 2000).
V0336 TrA    Min II = 11.1.
V0338 TrA    VB A (6.3mJ; B 10.3mJ, 7", 265deg, 2000).
V0344 TrA    VB B (A = NEXT STAR IN THE LIST; AB 13", 304deg, 2000).
V0345 TrA    VB A (B = PREVIOUS STAR IN THE LIST, 13", 304deg, 2000).
T     Tuc    P var. Max = 2410138 + 250.76d*E (JD2410000 - 14400);
T     Tuc    Max = 2414900 + 248.88d*E (JD2414400 - 22000);
T     Tuc    Max = 2432160 + 250.00d*E (JD2422900 - 35000);
T     Tuc    since JD2437700 - see Table.
U     Tuc    In the region of the Small Magellanic Cloud.
U     Tuc    SMS non-member.
U     Tuc    P var. Max = 2421190 + 258.12d*E (JD2412600 - 22000);
U     Tuc    Max = 2427487 + 262.83d*E (JD2422000 - 28000);
U     Tuc    Max = 2437808 + 257.70d*E (JD2428000 - 39150);
U     Tuc    since JD2440900 - see Table.
V     Tuc    In the region of the Small Magellanic Cloud.
V     Tuc    SMS non-member.
V     Tuc    The depth of Min II 0.11m.
W     Tuc    (k - b)2 = 0.09, Delta(S) = 7:. P var?
RR    Tuc    In the region of the Small Magellanic Cloud.
RR    Tuc    VB A (B 17m, 6", 90deg).
RV    Tuc    In the region of the Small Magellanic Cloud. VB.
SS    Tuc    In the region of the Small Magellanic Cloud. HV 1877.
SS    Tuc    Earlier was erroneously identifded with HV 1887.
SU    Tuc    In the region of the Small Magellanic Cloud. HV 1922.
SU    Tuc    According to [09980], alternatively may be identical to
SU    Tuc    HV 1920.
SX    Tuc    In the region of the Small Magellanic Cloud. VB (B 16m? P).
SY    Tuc    In the region of the Small Magellanic Cloud. Min II 15.4.
TV    Tuc    In the region of the Small Magellanic Cloud.
TV    Tuc    The variable's position in 2' to the north
TV    Tuc    of CPD -73deg 64 [09980] makes it impossible to identify
TV    Tuc    it with HV 2041.
TZ    Tuc    In the region of the Small Magellanic Cloud.
TZ    Tuc    SMS non-member.
TZ    Tuc    VB A (B 13m sp).
UW    Tuc    In the region of the Small Magellanic Cloud.
UW    Tuc    SMC non-member.
UX    Tuc    In the region of the Small Magellanic Cloud.
UX    Tuc    SMS non-member.In the neighbourhood OF 47 Tuc; probably
UX    Tuc    cluster non-member. P var. [Fe/H] = -1.8.
YY    Tuc    The elements need improvement; current elements with the
YY    Tuc    epoch from [07984] are given.
YY    Tuc    (k - b)2 = 0.03. Delta(S) = 8:.
AD    Tuc    In the region of the Small Magellanic Cloud.
AD    Tuc    SMS non-member. Delta(S) = 4.9.
AF    Tuc    In the region of the Small Magellanic Cloud. SMS
AF    Tuc    non-member.
AH    Tuc    In the region of the Small Magellanic Cloud. SMS
AH    Tuc    non-member. P var.
AI    Tuc    In the region of the Small Magellanic Cloud. SMS
AI    Tuc    non-member. In the region of the globular cluster NGC 362.
AI    Tuc    P var.
AK    Tuc    In the region of the Small Magellanic Cloud. SMS
AK    Tuc    non-member. P var.
AL    Tuc    In the region of the Small Magellanic Cloud. SMS
AL    Tuc    non-member.
AM    Tuc    The elements should be checked.
AM    Tuc    [Fe/H] = -1.82. Delta(S) = 9.9.
AO    Tuc    The elements need improvement. Delta(S) = 5.
AP    Tuc    In the region of the Small Magellanic Cloud. SMS
AP    Tuc    non-member.
AQ    Tuc    In the region of the Small Magellanic Cloud. SMS
AQ    Tuc    non-member.In the region of the globular cluster 47 Tuc.
AQ    Tuc    Min II 10.48.
AR    Tuc    In the region of the Small Magellanic Cloud. SMS
AR    Tuc    non-member.
AU    Tuc    In the region of the Small Magellanic Cloud. SMS
AU    Tuc    non-member.
AV    Tuc    In the region of the Small Magellanic Cloud. SMS
AV    Tuc    non-member.
BD    Tuc    In the region of the Small Magellanic Cloud. SMS
BD    Tuc    non-member.
BE    Tuc    In the region of the Small Magellanic Cloud.
BF    Tuc    In the region of the Small Magellanic Cloud. [A/H] = -0.7.
BG    Tuc    In the region of the Small Magellanic Cloud. SMS
BG    Tuc    non-member.
BH    Tuc    In the region of the Small Magellanic Cloud. VB A
BH    Tuc    (B 14.28m, 10" n).
BS    Tuc    (k - b)2 = 0.10.
BZ    Tuc    P var. Max = 2429849.448 + 127.78d*E (JD2410000 -
BZ    Tuc    35100) [03641]; Max = 2441193.541 +127.27d*E
BZ    Tuc    (JD2435100 - 43500) [A.M. van Genderen, AsAp Suppl 52,
BZ    Tuc    423, 1983]; since JD 2443500 - see Table.
CF    Tuc    In the region of the Small Magellanic Cloud. SMS
CF    Tuc    non-member. Soft X-ray source. Distortion
CF    Tuc    wave. Delta(m) = 0.057m [10065]. Min II 7.52.
DX    Tuc    Type RRC: is also possible.
EM    Tuc    Min II = 12.6.
EN    Tuc    Min II = 8.61.
EP    Tuc    Blazhko effect, P = 63d.
tet   Tuc    For the period of the main oscillation (A = 0.0132m) see
tet   Tuc    Table. Other instable frequences were also noted.
R     UMa    Maser (H2O).
S     UMa    S 1.5/6 e. P var. Max = 2398325 + 224.51d*E
S     UMa    (JD2394000 - 2405000); Max = 2405290 + 230.20d*E
S     UMa    (JD2405000 - 10500); Max = 2417530 + 223.96d*E
S     UMa    (JD2410500 - 23500); Max = 2426324 + 228.53d*E
S     UMa    (JD2423500 - 28800); since JD2428800 - see Table.
T     UMa    Maser (H2O).
W     UMa    ADS 7494 A (B 12.35m, 6.5", 44deg, 1963).
W     UMa    dI = 0.037P; Min II 8.43, dII = 0.028P.
W     UMa    Soft X-ray source. LX/Lbol = 1.7*10**(-4).
W     UMa    P var. Min I = 2420980.8093 + 0.333638880d*E
W     UMa    (JD2416000 - 21000); Min I = 2420980.8093 +
W     UMa    0.333636993d*E (JD2421000 - 33000) [01760];
W     UMa    Min I = 2435918.4169 + 0.33363832d*E (JD2433000 - 41000)
W     UMa    [05327]; since JD2441000 - see Table. The light curve shape,
W     UMa    including depths of minima, var. A moving wave with
W     UMa    Delta(m) = 0.025m y and P ~1100d [10067] was noted. A
W     UMa    flare (Delta(m) = 1.5m, lambda 3300 A,
W     UMa    delta(lambda) = 50 A, JD2438511.7,
W     UMa    delta(t) = 7 min) was announced [05788]. The system
W     UMa    contains gaseous streams, dark spots on the surface of
W     UMa    the components. H and K CaII emission.
Z     UMa    Usually 2 Max and 2 Min during a cycle.
RV    UMa    P var. Max = 2417861.434 + 0.4680618d*E
RV    UMa    (JD2417800 - 25000); Max = 2425053.675 + 0.4680654d*E
RV    UMa    (JD2425000 - 29000) [00188];
RV    UMa    Max = 2438459.945 + 0.468062d*E (JD2429000 - 40000) [03506];
RV    UMa    since JD2440000 - see Table. Blazhko effect, Pi = 92.12d
RV    UMa    (JD2436229 - 38114) [09835]. Pi var. [Fe/H] = -1.04;
RV    UMa    Delta(S) = 3.5.
RW    UMa    DI < 0.08P; Min II 10.34, DII = 0.10P.
RW    UMa    [Fe/H]A = -0.1, [Fe/H]B = -1.0. P var?
RW    UMa    Distortion wave, A = 0.11m V.
SU    UMa    The cycle of normal maxima 5d - 35d [09782, 03791].
SU    UMa    Three different mean values of the mean cycle of
SU    UMa    supermaxima change each other being active at different
SU    UMa    time intervals: P1 = 161.5d; P2 = 203.9d; P3 = 248.1d
SU    UMa    (P = 201.7d) [09276]. Porb = 2.06d/N (N = 26, 27, 28)
SU    UMa    or 3.1h. Surrounded by a faint halo (28' diameter) of soft
SU    UMa    X-ray sources.
SW    UMa    SB. Superior conjunction of the accretion disc
SW    UMa    T = 2445376.8601 + 0.0567433d*E [09836].
SX    UMa    P var strongly. Before JD2418800
SX    UMa    Max = 2416200.486 + 0.3071148d*E;
SX    UMa    Max = 2418800.213 + 0.3071345d:*E (JD2418800 - 22500)
SX    UMa    [00001]; Max = 2422653.5032 + 0.30711855d*E
SX    UMa    (JD2422500 - 26000) [10083]; Max = 2426400.418 +
SX    UMa    0.3071555d*E (JD2426000 - 29500); Max =
SX    UMa    2430000.250 + 0.3071301d*E (JD2429500 - 34000),
SX    UMa    Max = 2438508.751 + 0.3071363d*E (JD2434000 - 39000);
SX    UMa    since JD2441500 - see Table. [Fe/H] = -1.82,
SX    UMa    Delta(S) = 9.9.
SZ    UMa    mu alpha = -0.4853s, mu delta = +0.148".
TU    UMa    P var [03506]. [Fe/H] = -1.05, Delta(S) = 7.6.
TW    UMa    d = 0.002P; Min II 12.3:.
TX    UMa    Min II 7.13. P var. Min I = 2416426.801 + 3.063297d*E
TX    UMa    (JD2416000 - 22000); Min I = 2427926.492 + 3.063337d*E
TX    UMa    (JD2424200 - 30000); Min I = 2433440.431 + 3.063300d*E
TX    UMa    (JD2430000 - 38000) [09839]; since JD2438000 - see Table.
TY    UMa    P var, non-linear term: +6.4d*10**(-11)*E**2.
TY    UMa    dI = 0.05P, dII = 0.00P. The light curve shape var.
TY    UMa    12.10 <= Min I <= 12.14, 12.06 <= Min II <= 12.12.
UX    UMa    The shape of the eclipse light curve, the
UX    UMa    mean level of light outside eclipses, the depth of
UX    UMa    Min var. Deviations from the tabulated elements may
UX    UMa    reach  +-0.002d. Rapid brightness oscillations
UX    UMa    (28.54s <= P <= 30.02s) are sometimes observed [07304].
UX    UMa    Soft X-ray source.
UY    UMa    Min II 12.9.
VV    UMa    Min II 10.26. P var. Min I = 2439245.408 + 0.6873793d*E
VV    UMa    (JD2425600 - 40200) [09843]; Min I = 2440768.6280 +
VV    UMa    0.687367d*E (JD2440200 - 42700); since JD2442700 - see
VV    UMa    Table.
VX    UMa    Maser (H2O).
WX    UMa    Mu alpha = -0.4094s, mu delta = +0.955", VB B
WX    UMa    (A = BD +44deg 2051, dM2, 8.74m V; B 28", 133deg;
WX    UMa    common mu). Soft X-ray source. LX/LV = 0.095.
XY    UMa    Mu alpha = -0.0055s, mu delta = -0.175". P var.
XY    UMa    Non-linear term:  +2.77d*10**(-11)*E**2.
XY    UMa    The brightness outside eclipses var by 0.16m V. The depth
XY    UMa    of Min I is 0.48m - 0.67m, that of Min II is 0.19m.
XY    UMa    Migrating wave.
XZ    UMa    Min II 10.2. P var? Min = 2444986.445 + 1.2223105d*E
XZ    UMa    (JD2414990 - 45000); since JD2445000 - see Table.
AA    UMa    Min II 11.53, Max II 10.94. The elements should
AA    UMa    be checked.
AC    UMa    VB B (A = BD  + 65G671, 9.97m V, B-V = +0.50m; B 19",
AC    UMa    114deg, 1957). The chart in [08953] is wrong.
AD    UMa    Blazhko effect is possible. Pi = 35d - 40d,
AD    UMa    delta(A) = 0.2m.
AE    UMa    The fundamental mode P0 is given in the Table.
AE    UMa    P1 = 0.066527d, Pbeat = 0.293616d [09869].
AE    UMa    Max 10.86 - 11.10, Min 11.46 - 11.52.
AF    UMa    d = 0.05P.
AK    UMa    The elements need improvement.
AN    UMa    The epoch of Min for periodic (P = Porb) light variations
AN    UMa    with A <= 1m B is given. Min II is present. B - V = 0.0
AN    UMa    in Max light,  +0.5 during an eclipse; U - B = -1.1.
AN    UMa    Circular polarization in B light -9% to -35%; linear
AN    UMa    polarization 0% - 13% with a sharp Max near Max light.
AN    UMa    Rapid changes (A = 0.03m, f = 0.4 - 0.8 Hz). The mean
AN    UMa    light level and the light curve shape var. During the low
AN    UMa    state (B ~19m) the light variability with porb disappears,
AN    UMa    emission lines occur only during 10% of Porb, IR excess is
AN    UMa    noted. Soft X-ray source, var. Emissions of H, HeI,
AN    UMa    He II, NIII, FeII.
AW    UMa    dI = 0.06P:; Min II 7.08, dII = 0.11P.
AW    UMa    The light curve shape var.
AW    UMa    P var. Min I = 2442150.4385 + 0.43873234d*E
AW    UMa    (JD2438000 - 42200); since JD2442200 - see Table.
AX    UMa    P var. Max = 2435951.354 + 0.53510d*E (JD2435900 - 38200)
AX    UMa    [04375]; during JD2445000 - 45900 - see Table.
BE    UMa    d = 0.006P. Outside eclipses var
BE    UMa    14.8m <= B <= 16.0m (reflection effect). The depth of
BE    UMa    eclipses for lambda lambda 3330 - 3700 A is greater than
BE    UMa    4.3m,that for lambda lambda 5265 - 6005 A is 1.5m.
BG    UMa    Min II 10.93. Alternative type EW.
BH    UMa    Min II 12.3.
BI    UMa    Min II 15.8.
BK    UMa    [Fe/H] = -1.29, Delta(S) = 6.6.
BL    UMa    Min II 16.2.
BM    UMa    The depth of Min II 0.80m.
BN    UMa    [Fe/H] = -1.65, Delta(S) = 8.9.
BP    UMa    D <= 0.04P. The elements need confirmation.
CE    UMa    In the region of the cluster of galaxies Abell 1213.
CE    UMa    SN 1966 omicron?
CF    UMa    Groombridge 1830 B (A = BD +38deg 2285, V = 6.45m,
CF    UMa    B - V = +0.75m, G8 subdwarf, mu alpha =  + 0.339s,
CF    UMa    mu delta = -5.81"; B 2", 165deg). A possible flare on
CF    UMa    February 27, 1968. A brightening of the combined light by
CF    UMa    0.6m pg on April 27, 1939 [09881]. Maybe the object does
CF    UMa    not exist [09882].
CH    UMa    X-ray source 1E 1003 +67. LX/Lopt = 0.04.
CM    UMa    P var?
CQ    UMa    The epoch of Max in U and B light
CQ    UMa    coinciding with that of Min in V light is given.
CQ    UMa    A(U) = 0.06m, A(B) = 0.06m.
CR    UMa    The elements for Max in U light are given. In B and V
CR    UMa    bands no periodicity is apparent. A(U) = 0.03m.
CW    UMa    Mu = 0.27", P = 300deg.
DF    UMa    ADS 8242A (B 11.4m, 1.8", 60deg, 1960).
DF    UMa    The data for combined brightness are given in the Table.
DF    UMa    SB1, Porb = 1.033824d. Mu alpha =  +0.0131s,
DF    UMa    mu delta = -0.038". Besides rapid variations (V = 10.14m,
DF    UMa    Delta(V) = 0.05m), long term variations are possible.
DG    UMa    Blazhko effect is possible.
DK    UMa    Soft X-ray source, lg Lx/Lv = -3.5. [Fe/H] = -0.38.
DL    UMa    Eclipses with P = 0.42d [04706].
DM    UMa    SB1 (Porb = 7.492d).
DM    UMa    Min = 2444026.97 + 7.478d*E (1979 - 1982);
DM    UMa    1981 - 1984 - see Table. Two Min in the light curve in
DM    UMa    1981 - 1982.
DN    UMa    ADS 8347 ABC (A 7.2m vis; B 9.0m vis, 0.121", 142.0deg,
DN    UMa    1981.5; C 8.3m vis, 4.0", 42deg, 1980; D = BS 4561,
DN    UMa    A1pCrEuSr:, V = 7.03m, B - V = +0.01m, 63.0", 114deg).
DN    UMa    The range of combined brightness for the three components
DN    UMa    is given. It is not known which of the components varies.
DN    UMa    The component D was used as a comparison star.
DN    UMa    Min II 6.73, Min II - Min I = 0.504P.
GM    UMa    SB, discrepant Porb = 3.2424d.
HH    UMa    Type EW: is also possible.
HN    UMa    Type DSCT: is also possible.
HU    UMa    VB A (B = GSC 3014.0222 = L265-581, 24", 250 deg, common proper
HU    UMa    motion).
II    UMa    Type RR: is also possible.
LU    UMa    SB1, Porb = 13.572 d.
MM    UMa    Variable brown dwarf.
MS    UMa    MinII 12.50.
MT    UMa    MinII 12.09.
MV    UMa    SB.
NO    UMa    SB2?
NS    UMa    The period was improved in [045] compared to [025] using new data. VB A (B 12.5mV, 15", 48deg, 1999). The tabulated amplitude was influenced by the companion.
NT    UMa    A twice shorter period is possible [100].
NU    UMa    A twice shorter period is not excluded. VB (A 9.6mHp; B 11.9mHp, 1.1", 39deg, 1991).
NY    UMa    Porb = 42.628d.
OR    UMa    Min II = 12.4.
OT    UMa    Min II = 12.48.
OV    UMa    Min II = 11.10.
OX    UMa    Min II = 12.14.
OY    UMa    Min II = 13.3.
PP    UMa    Blazhko effect, P = 46d:.
PS    UMa    Min II = 12.78. MinII - MinI = 0.466P.
PU    UMa    Light elements for eclipsing variations in quiescence (19.1m - 21.2m) are tabulated.
PV    UMa    SB, Porb = 80.53d.
PW    UMa    Min II = 11.5.
PX    UMa    Slow variations on time scale of several days are also present.
PZ    UMa    Min II = 13.1.
QQ    UMa    Min II = 14.1.
QT    UMa    Min II = 11.70.
QV    UMa    Min II = 14.25.
V0337 UMa    Min II = 14.20.
V0342 UMa    The depth of MinII is 0.40 mag.
V0343 UMa    Min II = 14.35.
V0351 UMa    Porb = 0.0992d.
V0354 UMa    Min II = 11.12.
V0355 UMa    The white-dwarf pulsation period is tabulated, with an amplitude about 0.05m. Another period detected photometrically is 320 minutes or 344 minutes. Porb = 0.0573083d.
V0356 UMa    Min II = 13.0.
V0357 UMa    Min II = 12.8.
V0358 UMa    Min II = 12.45.
V0359 UMa    Multiperiodic.
V0360 UMa    Min II = 14.0.
V0362 UMa    Min II = 14.6.
V0363 UMa    Min II = 14.0.
V0364 UMa    Min II = 13.95.
V0365 UMa    Min II = 13.10.
V0366 UMa    Min II = 14.2 :.
eps   UMa    SB (P=4.15A). Interferometric binary? (0.053", 94.5deg,
eps   UMa    1975.4). In 1976 - 1983 attempts to resolve the binary
eps   UMa    interferometrically were not successful.
eps   UMa    In the UMa moving cluster; mu alpha = +0.0131s,
eps   UMa    mu delta = -0.010".
ups   UMa    ADS 7534 A (B 11.5m, 11.3", 295deg, common mu).
ups   UMa    mu alpha = -0.0382s, mu delta = -0.156". The light curve
ups   UMa    shape and A var.
R     UMi    H2O maser.
S     UMi    P var. Max = 2422604 + 321.9d*E (JD2413000 - 23000);
S     UMi    Max = 2432200 + 331.5d*E (JD2423000 - 32800);
S     UMi    Max = 2436080 + 322.5d*E (JD2433000 - 37000);
S     UMi    Max = 2439011 + 326.5d*E (JD2437000 - 41500);
S     UMi    since JD2441500 - see Table.
T     UMi    P var. Max = 2428332 + 315.48d*E (JD2416500 - 29500);
T     UMi    Max = 2436415 + 310.05d*E (JD2429500 - 37200);
T     UMi    Max = 2442389 + 315.5d*E (JD2437200 - 43600); since
T     UMi    JD2443600 - see Table.
U     UMi    P var. Max = 2416975 + 323.1d*E (JD2416500 - 21000);
U     UMi    Max = 2428804 + 331.3d*E (JD2421000 - 29780) [00001];
U     UMi    Max = 2429789 + 320.6d*E (JD2429780 - 34600) [00960];
U     UMi    Max = 2434600 + 331d*E (JD2434600 - 36300);
U     UMi    Max = 2437853 + 322.6d*E (JD2436300 - 39000); since
U     UMi    JD2439000 - see Table.
V     UMi    Mean brightness var with P2 = 760d.
W     UMi    Min II 8.66; d = 0.02P. P var? Non-linear term in the
W     UMi    elements is possible: -7.7d*10**(-10)*E**2.
X     UMi    P var? Max = 2424224 + 343d*E (JD2423800 - 25100)
X     UMi    [00684]; since JD2438100 - see Table.
RR    UMi    SB (Porb = 749.4d [09896]).
RT    UMi    Min II 10.86.
RU    UMi    Min II 10.20.
RZ    UMi    Min II 13.5.
SZ    UMi    Variability needs confirmation.
VV    UMi    MinII - MinI = 0.52P:.
VZ    UMi    Min II = 13.5.
WW    UMi    Min II = 12.55.
WX    UMi    Min II = 15.1.
WY    UMi    The ultraviolet-light amplitude is at least 1.6m.
WZ    UMi    Min II = 13.1.
AA    UMi    Min II = 12.68:.
AK    UMi    Type ELL with a twice longer period is not excluded.
alf   UMi    VB A (B 8.20m, F3V, 18.3", 218deg); SB1 (Porb = 10969d,
alf   UMi    E = 0.655 [09904]). P var. There is a non-linear term in
alf   UMi    the elements: +1.9877d*10**(-7)*E**2. The amplitude of
alf   UMi    light and radial velocity variation decreased in 1982.
alf   UMi    A(V) = 0.04m (1984).
gam   UMi    P var. Max = 2424301.78 + 0.14335d*E [10097]; Max =
gam   UMi    2427904.468 + 0.14335d*E [10098]. Elements given in the
gam   UMi    Table represent observations in 1964 - 1968. According to
gam   UMi    [09906] Vr var in 1922 with P = 0.108449d.
eps   UMi    VB A (B 12.5m, 76.9", 3deg). Min II 4.21.
S     Vel    Min II 7.83; d = 0.041P. P var? There is a non-linear term
S     Vel    in the elements given in the Table: +4.47d*10**(-9)*E**2.
W     Vel    P var. Max = 2415053 + 384.3d*E (JD2414600 - 17400);
W     Vel    Max = 2426080 + 399.9d*E (JD2422400 - 27300);
W     Vel    Max = 2429990 + 388.0d*E (JD2427300 - 30100);
W     Vel    Max = 2438328 + 398.7d*E (JD2430100 - 38800);
W     Vel    since JD2438800 - see Table. OH emission.
Y     Vel    P var. Max = 2415900 + 438.6d*E (JD2411500 - 15900);
Y     Vel    Max = 2419930 + 447.7d*E (JD2415900 - 19930);
Y     Vel    Max = 2425755 + 452.8d*E (JD2421600 - 27600);
Y     Vel    Max = 2434150 + 439.5d*E (JD2427600 - 34200);
Y     Vel    since JD2434200 - see Table.
Z     Vel    P var. Max = 2415445 + 435.96d*E (JD2415000 - 25100);
Z     Vel    Max = 2425462 + 417.99d*E (JD2425100 - 29700) [00960];
Z     Vel    since JD2429200 - see Table.
RR    Vel    Min II 10.9.
RS    Vel    P var. Max = 2410403 + 421d*E (JD2410400 - 16800)
RS    Vel    [09961]; since JD2415450 - see Table.
RU    Vel    VB A (B 12m sf). According to [00017],
RU    Vel    Max = 2414390 + 63d*E.
RW    Vel    P var. Max = 2413553 + 430.4d*E (JD2413500 - 18500);
RW    Vel    Max = 2420610 + 465.7d*E (JD2418500 - 25700); since
RW    Vel    JD2425700 - see Table.
RX    Vel    Min II 10.5.
RY    Vel    [A/H] = -0.3. P var. Max = 2440246.67 + 28.1270d*E
RY    Vel    (JD2419000 - 40250) [05366]; since JD2443900 - see Table.
SW    Vel    P var. Max = 2434872.95 + 23.473d*E - 3.75d*10**(-5)*E**2
SW    Vel    (JD2412500 - 35500) [09636]. Since JD2440700 - see Table.
SX    Vel    The light curve has double maximum. The epoch of
SX    Vel    the primary (second) maximum is given in the Table.
TT    Vel    Min II 10.7.
UW    Vel    In the region of the open cluster NGC 3033.
YZ    Vel    Min II 12.8; DII = 0.040P; Min II - Min I = 0.537P.
ZZ    Vel    Min II 10.0.
AA    Vel    Min II 9.9.
AC    Vel    Min II 9.11.
AF    Vel    (k - b)2 = 0.06. Blazhko effect is possible [10110].
AH    Vel    SB? [10111]. In the region of the open cluster
AH    Vel    Collinder 173.
AI    Vel    Mu = 0.11", P = 76deg; (k - b)2 = 0.23.
AI    Vel    Light oscillations with the period P0 given in the Table
AI    Vel    are superimposed by oscillations with P1 = 0.08620868d and
AI    Vel    twice smaller amplitude. According to [10112] P0 is
AI    Vel    constant, P1 is increasing.
AK    Vel    In the region of the open cluster Collinder 173.
AL    Vel    d = 0.072P.
AO    Vel    In the region of the open cluster Collinder 173.
AO    Vel    Min II 9.55:. There is apsidal line motion.
AO    Vel    There is a sinusoidal term in the elements given in the
AO    Vel    Table: +0.058d*sin(phi), where phi = 2pi(E - 5338)/11500,
AO    Vel    and E values are counted from JD2415810.66.
AO    Vel    Min II = 2424270.125 + 1.5845993d (E - 5338) -
AO    Vel    -0.058d*sin(phi); Min II - Min I = 0.792d - 0.116d*sin(phi).
AP    Vel    P1 = 2.19984d; P1/P0 = 0.703. M - m var (0.25P <= M - m <=
AP    Vel    <= 0.50P) [03710].
AQ    Vel    d = 0.05P. The depth of Min II 0.05m.
AS    Vel    Min II 8.4; Min II - Min I = 0.55P.
AT    Vel    d = 0.03P. In the region of the open cluster Collinder 173.
AU    Vel    In the region of the open cluster Collinder 173.
AV    Vel    In the region of the open cluster Collinder 173.
AW    Vel    In the region of the open cluster Collinder 173.
AX    Vel    The first overtone mode light variation elements with the
AX    Vel    period P1 are given in the Table; the amplitude of
AX    Vel    the first overtone mode light variation A1 exceeds
AX    Vel    that of the fundamental mode, A0:A1(V) = 1.5A0(V).
AX    Vel    For the fundamental mode P0 Max hel = 2443878.885 +
AX    Vel    3.673174d*E.
AX    Vel    P1/P0 = 0.706; M - m var: 0.24P <= M - m <= 0.50P:.
AY    Vel    Min II 9.7.
AZ    Vel    Min II 13.0. In the region of the open cluster
AZ    Vel    Collinder 173.
BB    Vel    P < 20d. In the region of the open cluster Collinder 173.
BC    Vel    Min II 12.3.
BD    Vel    d = 0.04P.
BE    Vel    Min II 12.5.
BF    Vel    The depth of Min II 0.04m.
BM    Vel    Min II 13.0. In the region of the open cluster NGC 2547.
BM    Vel    In the region of the open cluster Collinder 173.
BO    Vel    Min II 14.2.
BP    Vel    Min II 13.7.
BR    Vel    The shape of the light curve varies.
BT    Vel    Min II 14.8.
BU    Vel    Min II 10.96; Min II - Min I = 0.522P. In the region
BU    Vel    of the open cluster Collinder 173.
BV    Vel    In the region of the open cluster Collinder 173.
BW    Vel    Min II 14.3.
BX    Vel    In the region of the open cluster Tr 10.
BZ    Vel    Min II 10.4; Min II - Min I = 0.57P.
CK    Vel    D ~0.3d.
CL    Vel    Min II 13.4.
CR    Vel    d = 0.05P.
CS    Vel    [A/H] = 0.1. Possible member of the open
CS    Vel    cluster Ruprecht 79.
CU    Vel    The period of superhumps ~0.08d, A = 0.4m [10115].
CV    Vel    Min II 7.17.
CW    Vel    d = 0.024P. The depth of Min II 0.1m pg.
CZ    Vel    Min II 11.1.
DF    Vel    Min II 13.4.
DH    Vel    Min II 13.7.
DK    Vel    VB A (B 12.50m, 22", 315deg; C 16m, 10", 60deg).
DL    Vel    Min II 12.1.
DM    Vel    P = 123d?
DQ    Vel    Min II 11.0.
DS    Vel    Min II 10.8.
DT    Vel    (k - b)2 = 0.24.
DX    Vel    Min II 10.3. In the region of the open cluster Col 213.
EH    Vel    Min II 13.4.
EL    Vel    In the region of the open cluster Collinder 173.
EO    Vel    Min II 11.90, DII = 0.07P.
EO    Vel    Apsidal motion: Min II - Min I = 3.15d + 0.00003d*E.
EO    Vel    Min II = 2441716.75 + 5.32969d*E.
EP    Vel    In the region of the open cluster IC 2395.
ES    Vel    Min II 12.7.
ET    Vel    Min II 12.1.
EU    Vel    Min II 13.8.
EY    Vel    d = 0.04P:.
FM    Vel    Min II 12.9.
FS    Vel    Delta(S) = 10.
FT    Vel    Min II 10.5.
FW    Vel    Min II 10.0.
FX    Vel    Min II 10.5. The shape of the light curve varies.
FY    Vel    Min II 7.03. Type ELL? [06827].
FZ    Vel    VB A (B 12.08m, 24.2", 338deg).
GG    Vel    VB A (B 11.2m, 6", delta(alpha) = 0). P = 2.950432d?
GP    Vel    Min II 6.90. Min II - Min I = 0.55P.
GP    Vel    The shape of the light curve varies.
GP    Vel    There are probably long-period light
GP    Vel    oscillations: Min = 2442681.6 + 93.3d*E (A ~0.02m)
GP    Vel    [10051]. The period of X-ray pulses var: 282.8913s
GP    Vel    (1975.5) [10125]; 282.919s (1975.7) [10126]; 282.869s
GP    Vel    (1976.4), 282.838s (1976.9) [10127]; 282.80s (1978.9)
GP    Vel    [10128]; 282.745s (1979.3), 282.7874s (1980.3), 282.87s
GP    Vel    (1981.0) [10129]; 282.93s (1981.9 - 1982.9); 282.9306s
GP    Vel    (1983.2) [10078].
GV    Vel    In the region of the open cluster NGC 2660.
HU    Vel    Pulsar PSR 0833-45. In the nebula Vela SNR.
HU    Vel    Star M [08276]. The pulsed radiation varies in radio,
HU    Vel    optical and gamma rays with P = 0.089s.
HU    Vel    P var [10136 - 10139]: P = 0.089233318274s
HU    Vel    (JD2442553 - 680), P = 0.089234713929s (JD2442700 - 848),
HU    Vel    P = 0.089244007685s (JD2443654 - 676), P = 0.089245406487s
HU    Vel    (JD2443719 - 850) [10137]; P = 0.089256985348s
HU    Vel    (JD2444795.84) [10138].
HV    Vel    A member of the open cluster IC 2391.
HW    Vel    P = 0.26133d? A member of the open cluster IC 2391.
HX    Vel    VB A (B 7.1m, 0.3", 313deg, 1949); in the region
HX    Vel    of the open cluster IC 2395. Min II 5.50:.
HY    Vel    VB A (B 5.7m, 76.6"); a member of the open cluster IC 2391.
HY    Vel    Min II 4.90.
IL    Vel    A var (0.02m <= A <= 0.15m). Beat period 10.075d
IL    Vel    (Min A = 2443175.5 + 10.075d*E).
IM    Vel    VB A (B 9.73m, 3.3", 179deg, 1948).
IM    Vel    The double wave of light variations
IM    Vel    with rotation period Prot = 2.85204d and A = 0.03m is
IM    Vel    superimposed by oscillations with the periods
IM    Vel    P1 = 0.00812815d (A1 = 0.0043m), P2 = 0.00808206d
IM    Vel    (A2 = 0.0035m), P3 = 0.00810503d (A3 = 0.0008m), P4 =
IM    Vel    0.004052519d (A4 = 0.0009m), P5 = 0.004064065d
IM    Vel    (A5 = 0.0004m), P6 = 0.004041031d (A6 = 0.0004m),
IM    Vel    P7 = 0.00815128d (A7 = 0.0004m) [09208].
IN    Vel    P = 65 - 70d,
IP    Vel    VB A (B 11.2m V, 2.1", 200deg, 1929). P > 1.25d.
IQ    Vel    Min II 12.94; Min II - Min I = 0.500P.
IS    Vel    A(U) var: 0.005m <= A(U) <= 0.018m.
IT    Vel    Min II 7.08. P = 23.52d?
OQ    Vel    The type is doubtful.
V0360 Vel    Several close companions.
V0390 Vel    P = 89.9 d is also possible. SB, Porb = 499 d.
V0405 Vel    A twice shorter period is not excluded. VB (9", 346deg, 1976).
V0409 Vel    MinII - MinI = 0.28P.
V0420 Vel    Not CoD-45 05845 (identification suggested in [235]).
V0447 Vel    Min II = 11.91.
V0448 Vel    Min II = 11.96. P varies. dP/dt = -0.44 x 10^(-5) d/yr.
V0451 Vel    Min II = 7.49.
V0452 Vel    Min II = 11.01.
V0454 Vel    Min II = 7.65.
V0456 Vel    The depth of MinII is 0.45 mag.
V0457 Vel    Multiperiodic.
V0458 Vel    Multiperiodic.
V0459 Vel    Multiperiodic.
V0460 Vel    Blended. Multiperiodic.
V0461 Vel    After subtraction of the BE trends, EA variations 8.33m - 8.45m, MinII 8.44.
V0464 Vel    The depth of MinII is 0.30 mag.
V0465 Vel    Min II = 14.32.
V0467 Vel    Min II = 11.00:. The tabulated ephemeris is for eclipses. Pulsations: P = 0.432728d, amplitude 0.05m.
V0469 Vel    Min II = 9.51.
V0472 Vel    An atypical emission-line star with periodic brightness variations.
V0479 Vel    Min II = 9.22.
V0483 Vel    Min II = 8.25. VB AB (8.79m, 9.19m, 1.0", 53deg, 1991).
V0484 Vel    Min II = 9.91.
V0487 Vel    Cycles about 280d in maximum light with an amplitude up to 1m.
V0495 Vel    Min II = 10.47.
V0496 Vel    Min II = 9.21.
V0497 Vel    Min II = 9.63. VB AB (10.1m, 10.4m, 0.2", 150deg, 1991).
V0503 Vel    Min II = 8.98. VB AB (9.2m, 11.2m, 0.6", 107deg, 1945).
V0504 Vel    Min II = 18.20. Cluster non-member.
V0505 Vel    Min II = 18.54. Cluster non-member.
V0506 Vel    Min II = 17.60. Cluster non-member.
V0507 Vel    CMin II = 17.21. luster non-member.
V0508 Vel    Min II = 17.89. Cluster non-member.
V0509 Vel    Min II = 20.33. Cluster non-member.
V0510 Vel    Cluster non-member.
V0511 Vel    Min II = 20.00. Cluster non-member.
V0512 Vel    Min II = 17.84. Cluster non-member.
V0513 Vel    Min II = 19.29. Cluster non-member.
V0514 Vel    Cluster non-member.
V0516 Vel    A twice longer period is also possible. VB A (B 12.0m, 2", 29deg, 1945).
V0518 Vel    Min II = 12.14.
gam 2 Vel    VB A (B 4.22m, 41.3", 220deg).
gam 2 Vel    SB2 (Porb = 78.5002d [10119]). In HII region.
gam 2 Vel    T0 = 2433633.0 is the epoch of the conjunction where the
gam 2 Vel    O component is in front [10119].
lam   Vel    VB A (B 14.8m, 18.2", 137deg).
omi   Vel    A member of the open cluster IC 2391. P(VR) = 2.74d.
omi   Vel    P = 2.76d? SB1? The epoch of the light maximum is given.
omi   Vel    Close binary system?
R     Vir    P var. Max = 2381914 + 145.77d*E (JD2338900 - 2402000);
R     Vir    Max = 2402321 + 144.90d*E (JD2402000 - 18000);
R     Vir    Max = 2418268 + 145.48d*E (JD2418000 - 30000);
R     Vir    Max = 2430489 + 148.32d*E (JD2430000 - 34000);
R     Vir    Max = 2434193 + 144.63d*E (JD2434000 - 38500);
R     Vir    Max = 2438829 + 147.45d*E (JD2438500 - 43000);
R     Vir    since JD2443000 see Table. Maser (SiO).
S     Vir    P var. Max = 2399014 + 374.7d*E (JD2398600 - 2405000);
S     Vir    Max = 2412970 + 376.2d*E (JD2412000 - 23500, on average);
S     Vir    Max = 2423502 + 381.52d*E (JD2423500 - 23000); since
S     Vir    JD2433000 - see Table. Maser (H2O, SiO).
T     Vir    Maser (OH, H2O, SiO).
V     Vir    P var. Before JD2427000 Max = 2400467 + 250.17d*E;
V     Vir    Max = 2427225 + 246.54d*E (JD2427000 - 31500);
V     Vir    since JD2431500 - see Table.
W     Vir    The epoch of Min is given. P var.
W     Vir    Min = 2404151.168 + 17.2707d*E (JD2403000 - 23200);
W     Vir    Min = 2423200.837 + 17.2634d*E (JD2423200 - 29700);
W     Vir    since JD2429700 - see Table. The light curve shape var.
W     Vir    [Fe/H] = -1.03.
X     Vir    VB A (B 12m, dK4, 0.6', ~50deg). The brightenings
X     Vir    of 1871 and 1882 may be due to misidentification [01651].
Z     Vir    mu alpha = +0.0098S, mu delta = -0.120".
Z     Vir    P var. Max = 2409683 + 309.19d*E (JD2408000 - 18500);
Z     Vir    since JD2418500 - see Table.
RS    Vir    Maser (OH, H2O, SiO). P var. Max =2412592 + 351.29d*E
RS    Vir    (JD2412000 - 31000); since JD2431000 - see Table.
RT    Vir    Maser (OH, H2O, SiO). According to [10145], observations
RT    Vir    of 1970-1977 are not in agreement with the P value in the
RT    Vir    Table.
RU    Vir    P var? Max = 2425120 + 435.9d*E (JD2414000 - 31500); since
RU    Vir    JD2431500 - see Table.
RV    Vir    P var. Max = 2412272 + 268.39d*E (JD2412000 - 31500);
RV    Vir    since JD2431500 - see Table.
RX    Vir    VB (B 13.0m vis, 1.1", 107deg, 1939). According to
RX    Vir    photoelectric observations [06450, 08837], 8.72m - 8.81m V.
RX    Vir    Const? [06450].
SS    Vir    P var. Max = 2415910 + 352.75d*E (JD2415900 - 21500);
SS    Vir    Max = 2421913 + 361.7d*E (JD2421500 - 26500);
SS    Vir    Max = 2428359 + 350.12d*E (JD2426500 - 40000);
SS    Vir    since JD2440000 - see Table.
ST    Vir    P var. Max = 2425005533 + 0.4108494d*E (JD2422000 - 29100)
ST    Vir    [10146]; Max = 2436702.513 + 0.4108168d*E
ST    Vir    (JD2433000 - 39000) [03415]; since JD2439000 - see Table.
ST    Vir    Blazhko effect? Delta(S) = 0.8.
SU    Vir    P var. Max = 2415040 + 213.7d*E (JD2415000 - 19500);
SU    Vir    Max = 2419926 + 210.96d*E (JD2415000 - 31500);
SU    Vir    Max = 2437378 + 210.2d*E (JD2431500 - 38500);
SU    Vir    since JD2438500 - see Table.
SV    Vir    P var? The mean elements are given. Maser (H2O).
SZ    Vir    Possibly EW with a very small A.
TV    Vir    VB A (B P).
TW    Vir    Porb = 0.182666d [09430]. Variability of ellipsoidal
TW    Vir    character in H light: P = Porb/2, A(H) = 0.13m.
TW    Vir    X-ray source.
TX    Vir    VB A (B 15m, 0.3' P).
TY    Vir    [Fe/H] = -1.7.
TZ    Vir    P2 = 6900d is superimposed?
UU    Vir    [Fe/H] = -0.3. delta[S] = 0.7.
UW    Vir    d = 0.011P. P var. Min = 2419942.513 + 1.8106818d*E
UW    Vir    (JD2415000 - 34500); since JD2441000 - see Table
UY    Vir    d = 0.014P; Min II 8.1.
VV    Vir    Min II 12.2:.
VW    Vir    SN 1895 (NGC 4424).
XX    Vir    [Fe/H] = -1.5. Delta(S) = 9:.
YZ    Vir    [A/H] = -0.9.
AD    Vir    P var. Max = 2425259.259 + 0.5522109d*E
AD    Vir    (JD2419000 - 31000); since JD2431000 - see Table.
AF    Vir    P var. Max = 2429051.697 + 0.4838214d*E
AF    Vir    (JD2419500 - 36000); Max = 2436718.3758 +
AF    Vir    0.4838386d*E (JD2436000 - 37500) [10159];
AF    Vir    since JD2440000 - see Table. DM var.
AG    Vir    The depth of Min II up to 0.44m.
AG    Vir    The light curve shape and A var.
AG    Vir    dI = 0.03P:, dII = 0.66P. Min II - Min I = 0.512P.
AG    Vir    P var. Min = 2434487.4297 + 0.6426489d*E
AG    Vir    (JD2424500 - 34500); since JD2434500 - see Table.
AH    Vir    mu alpha = +0.0015S, mu delta = -0.111"
AH    Vir    ADS 8472 A (B 13.2m, 1.3", 17deg).
AH    Vir    The combined brightness is given,
AH    Vir    dI = 0.07P. The depth of Min II 0.53m, dII = 0.00P.
AH    Vir    The light curve shape var.
AH    Vir    P var. Min = 2434841.3963 + 0.40751843d*E
AH    Vir    (JD2425000 - 35000) [05222]; Min = 2435573.710 +
AH    Vir    0.40752192d*E (JD2435000 - 41400); Min =
AH    Vir    2441411.460  +  0.40753186d*E (JD2441400 - 44000);
AH    Vir    since JD2444000 - see Table.
AK    Vir    VB B (A = BD -17deg 3996; B 44", 286deg).
AL    Vir    P var [A/H] = -0.7.
AN    Vir    P2 ~1000d is superimposed.
AO    Vir    VB A (B 11.4m vis, 6.9", 321deg, 1956, common
AO    Vir    Vr). delta(M) is possibly in error because of the
AO    Vir    companion. P var. Max = 2413949  +  256.88d*E
AO    Vir    (JD2412900 - 21000); since JD2421000 - see Table.
AS    Vir    P var. The Table gives the mean elements valid after
AS    Vir    JD2425600. Blazhko effect? [03506].
AS    Vir    (k - b)2 = 0.08.
AT    Vir    P var. Max = 2426831.367 + 0.5258053d*E
AT    Vir    (JD2420500 - 35000) [00188]; since JD2435000 - see Table.
AT    Vir    (k - b)2 = 0.00, Delta(S) = 6.0.
AU    Vir    [Fe/H] = -1.84, Delta(S) = 10.1.
AV    Vir    Delta(S) = 5.5.
AW    Vir    Min II 11.67.
AX    Vir    Min II 10.24.
AY    Vir    Maser (H2O).
AZ    Vir    Min II 11.37.
BB    Vir    Blazhko effect?
BC    Vir    P var. Max = 2419922.289 + 0.56451468d*E
BC    Vir    (JD2419900 - 30100); the Table gives current elements.
BD    Vir    P var. Min = 2424971.720 + 2.548410d*E
BD    Vir    (JD2424900 - 32000); since JD2432000 - see Table.
BF    Vir    Min II 10.72. Total eclipses.
BF    Vir    P var. Min = 2416595.67 + 0.64057d:*E (JD2414000 - 19000);
BF    Vir    Min = 2440331.809 + 0.64057631d*E
BF    Vir    (JD2426000 - 41000); since JD2441000 - see Table.
BH    Vir    Min II 10.24. Distortion wave?
BH    Vir    (Delta(V) = 0.04m).
BN    Vir    P var. Max = 2419865.422 + 0.39127585d*E
BN    Vir    (JD2419800 - 28300); since JD2432600 - see Table.
BO    Vir    P var. Max = 2419513.388 + 0.52005916d*E
BO    Vir    (JD2419500 - 33000); since JD2433000 - see Table.
BQ    Vir    P var?
BS    Vir    [Fe/H] = -1.84. Delta(S) = 10.1.
BV    Vir    P var. Max = 2426070.488 + 0.4965803d*E
BV    Vir    (JD2419900 - 28500); since JD2436600 - see Table.
BW    Vir    P var. Max = 2420247.403 + 0.4706660d*E
BW    Vir    (JD2420200 - 26800); since JD2426800 - see Table.
CG    Vir    Min II 10.9.
CK    Vir    [Fe/H] = -2.0.
CM    Vir    d = 0.05P. P var. Min = 2425411.330 + 3.40167d*E
CM    Vir    (JD2423900 - 28400) [00001]; during JD2432200 - 34200 - see
CM    Vir    Table.
CS    Vir    The epoch of Max in B light is given.
CS    Vir    SB (Porb = 1618d). IR excess (4.8 mkm).
CU    Vir    ADS 9152 A (B 11.9m, G1V, 60", 212deg).
CW    Vir    The epoch of min is given.
CX    Vir    The depth of Min II 0.30m.
DK    Vir    According to [10189], P1 = 0.1162d, P2 = 0.1086d.
DK    Vir    (k - b)2 = 0.20.
DL    Vir    SB (Porb = 2286d).
DL    Vir    The spectrum shows the A-component of the eclipsing
DL    Vir    system and the G8III star around which the eclipsing
DL    Vir    system is orbiting.
DM    Vir    Min II 9.49. DII = DI.
DN    Vir    P >= 100d.
DT    Vir    Mu alpha = -0.044s, mu delta = -0.02". SB?
DT    Vir    Rotation period 1.535d [10014], A = 0.05m V.
DV    Vir    Blazhko effect?
EF    Vir    According to [04784], const?, 16.1m pg.
EP    Vir    IR excess (4.8 mkm).
EQ    Vir    SB; [Fe/H] = -0.08; mu alpha = -0.018s, mu delta = -0.09".
EQ    Vir    Min = 2441129.585 + 3.914169D*E + 0.0001803345d*E**2,
EQ    Vir    A = 0.10m V, M - m = 0.40P. Soft X-ray source,
EQ    Vir    lg FX/FV = -2.07.
EW    Vir    P >= 100d.
EX    Vir    P >= 100d.
EY    Vir    P >= 100d.
FF    Vir    The P value for magnetic field variations is given.
FG    Vir    ADS 8471 A (B 13.51m, 25", 352deg, 1909;
FG    Vir    C 11.85m, 74", 195deg, 1909).
FI    Vir    Mu alpha = +0.043s, mu delta = -1.22".
FL    Vir    VB AB (A = 0.76", P = 16A). Both components show flares?
FL    Vir    The range of combined brightness is given.
FL    Vir    Mu alpha = -0.118s, mu delta = +0.26".
FM    Vir    SB2, Porb = 38.324d.
FN    Vir    Mu alpha = -0.064s, mu delta = +0.28". SB?
FN    Vir    X-ray source, LX/Lbol = -3.55.
FO    Vir    Min II 6.67.
FQ    Vir    Deep Min II.
GG    Vir    Multiperiodicity, 0.023d <= P <= 0.083d, A <= 0.02m.
GH    Vir    P var.
GK    Vir    The secondary is a red dwarf (M0 - M6).
GL    Vir    Mu alpha = -0.087s; mu delta = +0.23".
GM    Vir    P ~1.6d/n.
GQ    Vir    Mu alpha = -0.045s, mu delta = -0.44".
GR    Vir    The depth of Min II 0.41m.
GU    Vir    P var. Max = 2439236.36 + 0.466562d*E
GU    Vir    (JD2438100 - 39300); during JD2441300 - 42600 - see Table.
LV    Vir    Type RR: is also possible.
MW    Vir    Type DSCTC: is also possible.
NN    Vir    Type EW: is also possible.
PS    Vir    MinII 12.2.
PT    Vir    MinII 13.54.
PU    Vir    MinII 11.68.
PY    Vir    MinII 10.04.
QU    Vir    MinII 12.03.
QX    Vir    MinII 12.6.
QZ    Vir    SB1 (Porb = 0.05881873d [09304]).
V0338 Vir    A twice longer or a twice shorter period is not excluded.
V0354 Vir    Blazhko effect, P = 59d: [026].
V0357 Vir    Blazhko effect? [422].
V0378 Vir    P = 0.268012d is also possible.
V0379 Vir    Porb = 0.061412d.
V0385 Vir    P = 0.447390d is also possible.
V0391 Vir    Min II = 13.6.
V0406 Vir    Quasi-periodic variations with a cycle about 0.39d. Porb = 0.05592d.
V0414 Vir    P = 0.492859d is also possible.
V0415 Vir    Min II = 10.32.
V0419 Vir    Blazhko effect, P = 65.69d.
V0439 Vir    Multiperiodic.
V0461 Vir    P = 0.153332d is also possible.
V0467 Vir    Min II = 9.69.
V0476 Vir    P varies?
V0492 Vir    P = 0.407024d is also possible.
V0503 Vir    Min II = 16.10.
V0533 Vir    P = 0.186684d is also possible.
V0546 Vir    Min II = 10.48.
V0551 Vir    Blazhko effect, P = 48d.
V0585 Vir    P varies. Before JD 2453700, Max = 2451961.85 + 0.60163d x E.
V0589 Vir    Min II = 14.20.
V0591 Vir    Min II = 12.38.
V0593 Vir    P = 0.186389d is also possible. Associated with an X-ray source.
V0594 Vir    Multiperiodic.
alf   Vir    The Table gives the epoch of Min for the ellipsoidal
alf   Vir    variability and Porb. The depth of Min II up to 0.08m.
alf   Vir    SB 2. e = 0.205 +- 0.004. Apsidal motion: Pi = 108a +- 5a.
alf   Vir    Pulsations: P var, P = 0.17378587d (1908 - 1956);
alf   Vir    since 1956 Max = 2445405.63 + 0.17378680d*E [10181]. A var.
alf   Vir    3 companions according to lunar occultation observations:
alf   Vir    3.1m, 0.0025"; 4.5m, 0.05"; 7.5m, 0.5". Soft X-ray source,
alf   Vir    LX/Lbol = 2.9*10**(-8).
psi   Vir    Binary? (lunar occultations).
R     Vol    P var. Max = 2415238 + 441d*E (JD2394100 - 2418800)
R     Vol    [10143]; since JD2422700 - see Table.
S     Vol    P var. Max = 2415042 + 397.6d*E (JD2415000 - 24200),
S     Vol    Max = 2428880 + 392.1d*E (JD2423000 - 28900),
S     Vol    Max = 2434113 + 401.7d*E (JD2428900 - 34900),
S     Vol    Max = 2434910 + 387.2d*E (JD2434900 - 39200);
S     Vol    since JD2439200 - see Table.
T     Vol    P var. Max = 2413135 + 189.8d*E (JD2413100 - 14600);
T     Vol    Max = 2416870 + 171.8d*E (JD2414600 - 16900);
T     Vol    Max = 2416870 + 176.8d*E (JD2416800 - 24400);
T     Vol    Max = 2424460 + 170.8d*E (JD2424400 - 27200);
T     Vol    Max = 2429925 + 182.3d*E (JD2427200 - 30000);
T     Vol    since JD2440000 see Table.
RX    Vol    P < 20d?
ST    Vol    SP component of a very close pair.
SV    Vol    The shape of the light curve varies.
TX    Vol    Min II 10.5. P var. Min I = 2416789.869 + 5.38845d*E
TX    Vol    (JD2415100 - 26000), Min I = 2431150.345 +
TX    Vol    5.3887d*E (JD2426000 - 31400), Min I =
TX    Vol    2433542.609 + 5.388d*E (JD2431400 - 33600)
TX    Vol    [00001]; since JD2433600 see Table.
YZ    Vol    A twice shorter period is not excluded.
AD    Vol    VB A (B 14.8mpg, 19", 260deg, 2000).
AH    Vol    Min II = 11.8.
AL    Vol    P0 is tabulated, P1 = 0.38521d.
R     Vul    P var. Max = 2400169 + 138.3d*E (JD2400100 - 02700),
R     Vul    Max = 2402779 + 136.76d*E (JD2402700 - 19800),
R     Vul    Max = 2419880 + 137.45d*E (JD2419800 - 24400),
R     Vul    Max = 2424413 + 136.76d*E (JD2424400 - 28500
R     Vul    [00960]; Max = 2429331 + 135.9d*E (JD2428500 - 32000)
R     Vul    [00001]; since JD2432000 see Table.
S     Vul    In the region of the open cluster C 1947 + 272 [10123].
S     Vul    P var. Max = 2401772 + 67.37d*E (JD2401760 - 6400),
S     Vul    Max = 2408180 + 67.70d*E (JD2408170 - 14950),
S     Vul    Max = 2415285 + 68.26d*E (JD2415300 - 22800),
S     Vul    Max = 2423468 + 67.72d*E (JD2423450 - 27200),
S     Vul    Max = 2428227 + 68.18d*E (JD2428220 - 31300)
S     Vul    [00761]; Max = 2432775 + 67.51d*E (JD2431300 - 34500)
S     Vul    [10148]; Max = 2437150 + 68.66d*E
S     Vul    (JD2436800 - 39600), Max = 2441507 + 67.344d*E
S     Vul    (JD2439600 - 43000) [10124]; since JD2443000 see Table.
S     Vul    [A/H] = 0.1.
T     Vul    P var. Max = 2419372.151 + 4.435589d*E (JD2409880 - 34000);
T     Vul    since JD2434000 see Table.
V     Vul    Min II 8.65. P var. Min I = 2414912.9 + 74.96d*E
V     Vul    (JD2414900 - 20840),  Min I = 2420909.8 + 75.686d*E
V     Vul    (JD2420900 - 24810), Min I = 2425072.9 + 76.344d*E
V     Vul    (JD2425050 - 30000), Min I = 2430023.5 + 75.957d*E
V     Vul    (JD2430000 - 32500) [10149]. Study of period variation and
V     Vul    changes of Min II by Min I see also in [00767, 010150].
W     Vul    In the region of the open clusters NGC 6882, NGC 6885.
X     Vul    P var. Max = 2420636.337 + 6.319301d*E (JD2417000 - 34000)
X     Vul    [00768]; since JD2435000 - see Table.
Z     Vul    VB A (B 12.0m, 13", 359deg). Min II 7.58. P var. Min I =
Z     Vul    2425456.117 + 2.454926d*E (JD2413200 - 37000)
Z     Vul    [00063]; since JD2437000 - see Table.
RS    Vul    Min II 6.86; Min II - Min I = 0.508P.
RU    Vul    A var. P var. Max = 2416266 + 155.95d*E
RU    Vul    (JD2415000 - 36000), Max = 2436779 + 150.7d*E
RU    Vul    (JD2436000 - 38800), Max = 2438855 + 153.4d*E
RU    Vul    (JD2438800 - 41620), Max = 2441193 + 138.5d*E
RU    Vul    (JD2441620 - 42600); since JD2442600 - see Table.
RX    Vul    P var. Max = 2420301 + 438d*E (JD2418900 - 22500)
RX    Vul    [04018]; since JD2424700 - see Table.
RZ    Vul    Slow variations of mean brightness with P = 1410D and
RZ    Vul    A = 2m are superimposed by fluctuations with the cycle
RZ    Vul    40 - 100d and A up to 1m.
SU    Vul    In the region of the open cluster NGC 6882, NGC 6885.
SV    Vul    [Fe/H] = 0.23. P var. There is a nonlinear term in the
SV    Vul    elements given in the Table: -0.0001814d*E**2.
SX    Vul    In the region of the open cluster NGC 6940.
UU    Vul    The co-ordinates are wrong?
UU    Vul    [10156].
VV    Vul    Min II 12.1; d = 0.026P. P var. Min I = 2416670.527 +
VV    Vul    3.411224d*E (JD2416600 - 27500) [00134];
VV    Vul    since JD2426000 - see Table.
VW    Vul    Porb = 0.0731d [10160].
VY    Vul    Min II 14.4:.
WW    Vul    There is quasi-periodicity in light minima with the cycle
WW    Vul    404d.
XZ    Vul    Min II 11.4. P var. Min I = 2426477.525 + 3.0895116d*E
XZ    Vul    (JD2416900 - 36000) [04427]; since JD2436000 - see Table.
AB    Vul    The depth of Min II 0.02m.
AD    Vul    Min II 0.010P.
AF    Vul    Min = 2436545.23  +  0.954d*E (JD2436200 - 900) [03148].
AR    Vul    In the region of the open cluster Stock 1.
AT    Vul    Min II 9.3; d = 0.02P.
AW    Vul    Min II 10.9; d = 0.020P.
AX    Vul    d = 0.018P.
AY    Vul    d = 0.020P. P var. Min hel = 2436128.388 + 2.4124239d*E
AY    Vul    (JD2418500 - 40700); since JD2440700 - see Table.
AZ    Vul    Min II 11.9.
BB    Vul    In the region of the open cluster NGC 6940.
BE    Vul    VB A (BC 11.92m, 50", 320deg). Min II 9.90. P var.
BE    Vul    Min I = 2426144.490 + 1.55205d*E
BE    Vul    (JD2426140 - 28880), Min I = 2430698.203 +
BE    Vul    1.5520442d*E (JD2430690 - 34660), Min I =
BE    Vul    2435340.373 + 1.552052d*E (JD2435340 - 40070);
BE    Vul    since JD2440100 - see Table.
BF    Vul    Elements given in the Table represent well only the bright
BF    Vul    maxima. The fainter maxima are represented by the elements:
BF    Vul    Max = 2427731 + 95.4d*E.
BI    Vul    Min II 14.86. P var? Min I = 2424759.70 + 0.251828d*E
BI    Vul    [00193]; since JD2444750 - see Table.
BN    Vul    Delta(S) = 7. P var. Max = 2414815.759 + 0.5941295d*E
BN    Vul    (JD2414000 - 30000) [00388]; Max = 2434244.333 +
BN    Vul    0.59412538d*E (JD2430000 - 36000) [00616];
BN    Vul    Max = 2438265.386 + 0.59412763d*E (JD2436000 -
BN    Vul    41000) [09009]; since JD2441000 - see Table.
BO    Vul    Min II 10.6. P var. Min I = 2429984.332 + 1.9459123d*E
BO    Vul    (JD2415000 - 30000) [00007]; Min I = 2432379.766 +
BO    Vul    1.9459206d*E (JD2427000 - 35000), since
BO    Vul    JD2435300 - see Table.
BP    Vul    Min II 10.5.
BS    Vul    Min II 11.10.
BT    Vul    d = 0.03P; Min II 12.3.
BU    Vul    P var. Min = 2431006.204 + 0.5689904d*E
BU    Vul    (JD2426500 - 31100) [00001];  since JD2433500 - see Table.
BV    Vul    S 6.5/6-.
BW    Vul    P var. Max = 2424000.171 + 0.20102229d*E
BW    Vul    (JD2424000 - 26500), Max = 2426500.079 +
BW    Vul     + 0.20102933d*E (JD2426500 - 31500), Max =
BW    Vul    = 2432000.054 + 0.20103513d*E (JD2431500 - 41000);
BW    Vul    since JD2441000 - see Table.
CD    Vul    Min II 11.9.
CK    Vul    Max 2331186:. Connected with nebulae. Type NR?
CS    Vul    Min II 13.6.
DR    Vul    Min II 9.19; DII = 0.132P.
DR    Vul    There is apsidal motion with the period 37.8 years.
DR    Vul    Elements given in the Table contain supplementary
DR    Vul    terms: -0.07165d*sin(0.05863deg*E) - 0.00269d*
DR    Vul    *sin(0.11726deg*E).
DR    Vul    Min II = 2440301.7934 + 2.2508645d*E + 0.07165d*
DR    Vul    *sin(0.05863deg*E) - 0.00269d*sin(0.11726deg*E).
DR    Vul    P var? [10185]. The depth of minima varies.
DY    Vul    VB A (B 13.0m V, 14", 300deg).
EH    Vul    P var. Max = 2429609 + 185d*E (JD2429600 - 30600);
EH    Vul    since JD2430800 - see Table.
EP    Vul    S 6.5/5.
EQ    Vul    Min II 12.5; Min II - Min I = 0.31P; DII = 0.050P,
EQ    Vul    dII =  0.010P.
ER    Vul    P var. Min I = 2440182.2593 + 0.69809510d*E
ER    Vul    (JD2433100 - 40200) [08592]; since JD2440100 - see Table.
ER    Vul    7.35m <= Min II <= 7.44m. The shape of the light
ER    Vul    curve and depths of minima vary.
ES    Vul    VB A (B 10.1m, 1.6", 126deg).
ET    Vul    [A/H] = -0.4. P var. Max = 2425110.63 + 54.33d*E
ET    Vul    (JD2422900 - 26600), Max = 2432875.80 + 54.33132d*E
ET    Vul    (JD2432700 - 35430), Max = 2438656.99 + 53.81d*E
ET    Vul    (JD2436050 - 39035), Max = 2439253.55 + 54.24d*E
ET    Vul    (JD2439035 - 40990) [10168]; since JD2441900 - see Table.
EU    Vul    Min II 13.3.
EV    Vul    Min II 11.9. P var. Min I = 2428750.459 + 2.822084d*E
EV    Vul    (JD2428400 - 36400) [04027]; Min I = 2436748.37 +
EV    Vul    2.82220d*E (JD2436380 - 750) [03732]; since
EV    Vul    JD2441500 - see Table.
EX    Vul    d = 0.03P.
EY    Vul    The depth of Min II 0.05m.
FG    Vul    In the region of the open cluster NGC 6940. Star 120.
FG    Vul    The epoch of light minimum is given.
FH    Vul    P var. The elements given in the Table are valid since
FH    Vul    JD2436000.
FK    Vul    Blazhko effect.
FM    Vul    Min II 13.0.
FN    Vul    d = 0.02P; Min II 14.2.
FP    Vul    Min II 15.6.
FQ    Vul    Min II 12.9. Apsidal motion with P = 280 years. Correction
FQ    Vul    of mispints in [04248] see in [04244].
FR    Vul    Probably the period must be doubled.
FS    Vul    Min II 15.2.
FU    Vul    sp component of a close pair.
FW    Vul    Min II 12.9.
FY    Vul    sp component of a close pair. Cycle 30 - 70d [04027].
FZ    Vul    Min II 13.9.
GG    Vul    P var. Max = 2427681.0 + 106.5d*E (JD2427500 - 28850);
GG    Vul    since JD2428850 - see Table.
GH    Vul    P = 2.5d?
GI    Vul    Min II 13.8.
GK    Vul    Red.
GN    Vul    Min II 12.4; d = 0.04P.
GO    Vul    Min II - Min I = 0.515P. The depth of Min II 0.03m.
GP    Vul    Min II 11.2; Min II - Min I = 0.48P.
GQ    Vul    nf component of a close triple group of stars.
GQ    Vul    P var. Max = 2434399.825 + 12.647241d*E (JD2426100 - 38000)
GQ    Vul    [04414]; since JD2444600 - see Table.
GR    Vul    Min II 13.3. The chart in [04244] is wrong.
GT    Vul    Min II 15.8.
GU    Vul    Min II 12.2.
GV    Vul    Probably the period must be doubled. Probably the period
GV    Vul    must be doubled.
HI    Vul    Min II 12.6.
HP    Vul    The depth of Min II 0.04m.
HS    Vul    Min II 14.2.
HU    Vul    Blazhko effect?
HV    Vul    P var. Max = 2437165.449 + 0.419906d*E (JD2437100 - 38670);
HV    Vul    since JD2438670 - see Table. Blazhko effect?
HW    Vul    P var. Max = 2429077.0 + 75.44d*E (JD2427190 - 29080),
HW    Vul    Max = 2429077.0 + 73.94d*E (JD2429070 - 32470);
HW    Vul    since JD2432350 - see Table.
IU    Vul    P var. Max = 2434656 + 320.2d*E (JD2432700 - 37860) [04427];
IU    Vul    since JD2437860 - see Table.
IW    Vul    Min II 13.1.
KN    Vul    Min II 13.4.
KO    Vul    Red.
KS    Vul    Very red.
LT    Vul    Multiperiodicity: P1 = 0.109414d, A1(V) = 0.0234m;
LT    Vul    P2 = 0.11094d, A2(V) = 0.0074m; P3 = 0.1215d,
LT    Vul    A3(V) = 0.0070m (JD2444054 - 096) [10173];
LT    Vul    P1 = 0.109621d, A1(B) = 0.0340m; P2 = 0.093528d,
LT    Vul    A2(B) = 0.0136m (JD2444071 - 465) [10193].
LU    Vul    Nova Vul 1968 N2.
LV    Vul    Nova Vul 1968 N1. VB A (B 18m, 6", 115deg).
LW    Vul    Min II 16.3.
MN    Vul    Min II 16.1; Min II - Min I = 0.518P; DII = 0.10P.
MO    Vul    Min II 14.8. P var?
MR    Vul    P2 = 111.0d?
MT    Vul    Multiperiodicity:
MT    Vul    P2 = 119.93d (A2 = 0.3m), P3 = 25.02d (A3 = 0.4m:).
MX    Vul    P = 181.8d?
NO    Vul    Min II 14.1.
NS    Vul    VB A (B 8.8m, A0, 0.73", 273deg, 1978.6),
NS    Vul    The range of combined light variation is given.
PS    Vul    VB A (B 10.0m, 0.4", 105deg, 1980.0); SB2.
PT    Vul    P1 = 256.12714s (A1 = 1.14%), Max1 =
PT    Vul    2445166.660914 HJED; P2 = 256.33205s (A2 = 1.09%),
PT    Vul    Max2 = 2445166.659424 HJED; P3 = 128.11496s (A3 = 0.37%),
PT    Vul    Max3 = 2445166.660024 HJED. mu = 0.1508", P=1.6deg.
PU    Vul    Pre-outburst SP M4 (1958). Gradual light increase in
PU    Vul    1977 - 79 up to 8.7m V; in 1979 A = 0.29M V,
PU    Vul    Min I = 2443943.39 + 78.12d*E [10197]. In the max of 1979
PU    Vul    Sp F5Ia - F8-9I. In February 1980 an abrupt light decrease
PU    Vul    started; the star reached V = 13.65m by early September.
PU    Vul    By September, 1981 the star recovered from the deep Min of
PU    Vul    500d duration. During the 1980 - 81 minimum Sp M5 with TiO
PU    Vul    bands, emissions of Halpha, NaD, [OII], FeII, rare earths.
PU    Vul    In 1982 - 84 8.35m - 8.87m V, Sp became F again. Simetimes
PU    Vul    Halpha, Hbeta emissions have been detected, often
PU    Vul    with P Cyg profiles.
V0398 Vul    Not identical to IRC+30416 = NSV 12861.
V0469 Vul    Red, despite Sp B in the literature.
V0477 Vul    Multiperiodic, P2 = 0.0644149d.
V0479 Vul    Multiperiodic, P2 = 0.10114d.
V0491 Vul    MinII - MinI = 0.327P. VB AB (10.9m, 11.1m, 0.6", 223deg, 2010).
V0495 Vul    MinII - MinI = 0.544P.
V0498 Vul    Superhumps: P = 0.05990d. A possible cycle between outburtsts is about 1000d.
V0507 Vul    Period varies. Light elements for JD 2454200-2455150 are tabulated. For JD 2452750-2453950, Max = JD 2453169.815 + 0.336042 x E.
