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.
PV    Aps  MinII - MinI = 0.75P.
OV    Aqr  A twice longer period is not excluded.
V1707 Aql  VB A (B 13.9m, 18", 166deg, 2000). The companion influenced the tabulated amplitude.
V1710 Aql  Epoch of Max is given. Continuous periodic brightness variations.
V1711 Aql  The identification with V1419 Aql in [064] is wrong.
V1719 Aql  A twice longer period is not excluded.
V0883 Ara  MinII - MinI = 0.44P.
V0560 Aur  VB (A 9.2m; B 9.6m, 0.9", 37deg, 1991).
V0574 Aur  VB A (B 15.0mV, 11", 72deg, 2000).
V0579 Aur  VB A (B 15.4mV, 8", 133deg, 1999).
HQ    Boo  VB A (B 15.0mV, 24", 21deg, 1998). The tabulated amplitude can be influenced by the companion.
V0377 CMa  A twice shorter period is not excluded.
V0383 CMa  Identification and type suggested in [055].
V0388 CMa  MinII - MinI = 0.61P. VB (A 9.1m; B 9.1m, 3", 150deg, 1991).
DL    CMi  A twice shorter period is not excluded.
CR    Cap  The first-overtone period is tabulated. P0 = 0.47203d, Delta(m)1/Delta(m)0 = 1.5.
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).
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.
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.
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 [241]. The data in [004] are actually for GSC 4252.00821.
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.
FO    Cha  VB A (B 10.75m, 12", 161deg, 2000).
DK    Cir  MinII - MinI = 0.75P.
AW    Col  MinII - MinI = 0.79P.
MT    Com  Small-amplitude pulsations with characteristic periods 1344, 1236, 668 seconds.
V0731 CrA  Large scatter on the light curve.
EP    Cru  MinII - MinI = 0.62P.
EQ    Cru  MinII - MinI = 0.48P.
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).
OX    Del  A twice longer period is not excluded.
NO    Dra  A twice shorter period is not excluded. VB (8.4mHp, 9.6mHp, 0.1", 128deg, 1991).
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.
AV    For  VB AB (A 8.8m; B 10.0m, 1.5", 24deg, 1962; C 10.8m, 35", 102deg, 1931).
V0383 Gem  VB A (B 15.2mV, 12", 212deg, 1998; more companions at larger distances). The tabulated amplitude was influenced by the companions.
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.
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.
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.
CQ    Ind  MinII - MinI = 0.33P.
V0457 Lac  A twice shorter period is not excluded.
HM    Leo  Porb = 0.1868d.
HQ    Leo  The tabulated amplitude was probably influenced by a companion in 35" np.
AM    Lep  VB B (A = HR 1696, 4.45m, B8V; B 12", 337deg, 1998).
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.
AT    Men  LMC non-member.
AU    Men  LMC non-member.
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).
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).
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.
DZ    Oct  Blazhko effect, P=36.8d.
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).
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].
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.
V0732 Per  A twice shorter period is not excluded.
CZ    Phe  The first-overtone period is tabulated. P0 = 0.56680d, Delta(m)1/Delta(m)0 = 1.9.
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).
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).
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.
DK    Pyx  MinII - MinI = 0.29P.
DN    Pyx  A twice shorter period is not excluded.
VY    Ret  MinII - MinI = 0.75P.
V0366 Sge  O'Connell effect.
V0370 Sge  MinII - MinI = 0.38P.
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.
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.
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).
V0493 Sct  MinII - MinI = 0.75P.
V0413 Ser  Apsidal motion, P(MinII) = 2.259735d. VB(9.1m, 9.1m, 0.3", 215deg, 1991).
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.
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).
NT    TrA  MinII - MinI = 0.57P.
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.
VV    UMi  MinII - MinI = 0.52P:.
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]).
V0338 Vir  A twice longer or a twice shorter period is not excluded.
YZ    Vol  A twice shorter period is not excluded.
AD    Vol  VB A (B 14.8mpg, 19", 260deg, 2000).