Документ взят из кэша поисковой машины. Адрес оригинального документа : http://sai.msu.ru/groups/cluster/gcvs/gcvs/iii/remark.txt Дата изменения: Thu Mar 24 19:17:40 2016 Дата индексирования: Sun Apr 10 00:08:31 2016 Кодировка: Поисковые слова: m 5

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 [79064]. Not CPD-38 03763 (identification suggested in [79091]).
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? [80233].
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