V0769 And | VB B (A 16.8mV, B 16.9mV; AB 6", 37deg, 1998). The magnitudes in the Table were influenced with the companion.
V0770 And | Multiperiodic.
V0390 Aps | Distorsion wave: P = 2.84455d.
V0393 Aps | Period varies.
V0394 Aps | VB A (B 7", 340deg, 2000).
V0366 Aqr | Multiperiodic.
V0367 Aqr | Double-mode pulsations. First overtone: see the Table. P0 = 0.485897d. P1/P0 = 0.7432.
V0368 Aqr | P1 is presented in the Table. P0 =0.481835d. P1/P0=0.7443.
V0369 Aqr | P1 is presented in the Table. P0 = 0.590458. P1/P0 = 0.7446.
V0370 Aqr | P1 is presented in the Table. Fundamental mode: Max = 2454700.685 + 0.532434d x E. P1/P0 = 0.7469.
V0371 Aqr | Double-mode pulsation. The period in the Table is for the fundamental mode. P1 = 0.0624379d. P1/P0 = 0.7748.
V0373 Aqr | Double-mode pulsation. The period in the Table is for the first overtone. P0 = 0.554570d. P1/P0 = 0.7456.
V0375 Aqr | Double-mode pulsation. The period in the Table is for the first overtone. P0 = 0.479278d. P1/P0 = 0.7443.
V0379 Aqr | Double-mode pulsation. The period in the Table is for the first overtone. P0 = 0.395471d. P1/P0 = 0.7459.
V0380 Aqr | Double-mode pulsation. The period in the Table is for the first overtone. P0 = 0.4900d. P1/P0 = 0.7429.
V0381 Aqr | Period varies.
V0383 Aqr | Period varies strongly.
V1834 Aql | A period about 230d is superposed.
V1837 Aql | The period for the first overtone is given in the Table. Second overtone: Max = 2453729.40+ 1.01121d x E. P1 given in the Table. P2/P1 = 0.8040.
V1844 Aql | Multiperiodic.
V1853 Aql | VB (2"). Other possible periods: 0.66579d or 0.49934d. RRC type with P = 0.24967d is also possible.
V1861 Aql | VB (3").
V1876 Aql | The one-day alias, P = 0.058916d, is also possible.
V1877 Aql | P = 0.30306d is also possible.
V1878 Aql | VB A (B 4", 24deg, 1999).
V1880 Aql | P = 0.42243d is also possible.
V1881 Aql | Blazhko effect.
V1883 Aql | The one-day alias, P = 0.109205d, is also possible.
V1886 Aql | Period varies.
V1889 Aql | Multiperiodic. P2 = 0.1004498d.
V1898 Aql | P = 0.4102d is also possible.
V1000 Ara | VB A (B 9" p).
V1011 Ara | Period varies.
V1027 Ara | VB A (B 14.0m, 12", 51deg, 2000). The magnitudes in the Table were influenced by the companion.
V1042 Ara | VB A (B 12.5m, 8.5", 329deg, 2000).
DO    Cap | Period varies strongly.
DQ    Cap | Blazhko effect [81005].
V1292 Cas | P = 0.311336d is also possible.
V1293 Cas | Oscillations outside MinI, amplitude 0.04mV, periods 0.12d and 0.045d.
V1004 Cep | MinII - MinI = 0.22P.
V1009 Cep | Multiperiodic.
V0756 CrA | Double-mode. P0 is given in the Table; P1 = 0.0821611d, P1/P0 = 0.7665.
V2669 Cyg | The one-day alias, P = 0.334285d, is also possible.
V2690 Cyg | Porb = 0.492d.
V2693 Cyg | VB B (A 14.08m; B 2.5" sf).
V2699 Cyg | Multiperiodic.
V2700 Cyg | Multiperiodic, 3 main frequencies.
V2709 Cyg | Possible non-radial pulsations of a white dwarf. P2 = 0.017070d.
V2737 Cyg | O'Connell effect.
V2740 Cyg | O'Connell effect.
V2760 Cyg | VB (3"). P=1.4088d is also possible.
V2761 Cyg | O'Connell effect.
V2762 Cyg | Porb = 12.7d; Pspin = 358.6s.
V2764 Cyg | O'Connell effect.
V2777 Cyg | O'Connell effect.
V2786 Cyg | Blazhko effect.
V2797 Cyg | P = 1.656d is also possible.
V2800 Cyg | The light curve shape varies.
V2813 Cyg | MinII - MinI = 0.64P.
V2838 Cyg | Multiperiodic? P2 = 0.13564d is possible [81213].
V0534 Dra | VB A (14.4mV; B 16.1m*, 5", 359deg, 2000).
VY    Equ | Double-mode pulsations. Fundamental mode: see the Table. First overtone: P1 = 0.1407792d. P1/P0 = 0.7978.
ER    Gru | Blazhko effect.
ES    Gru | Period varies?
EX    Gru | The coordinates in [81005] are wrong.
V1440 Her | P2 = 0.291982d. Mode identification is unclear.
V1441 Her | Multiperiodic.
V1446 Her | VB A (B 3", 133deg, 2000). The magnitudes in the Table were influenced with the companion.
DI    Ind | Type EW with a twice longer period is not excluded.
DQ    Ind | Type DSCT: with P = 0.1163d is also possible.
DS    Ind | Period varies strongly.
V0485 Lac | O'Connell effect.
V0493 Lac | EW type with a twice longer period is also possible.
V0514 Lac | A twice longer period is also possible.
V0524 Lac | VB A (B 4", 112deg, 1998). Double-mode pulsation. The other period is 0.101399d.
V0529 Lac | VB A (B 5", 297deg, 1998).
V0556 Lac | A twice longer period is also possible.
V0568 Lac | P = 0.12351d is also possible.
V0600 Lac | VB A (B 4.5", 207deg, 1998).
V0607 Lac | Near the galaxy 2MASX J22525476+5235101.
V0639 Lac | A twice longer period is also possible.
V0651 Lac | RRC type with P = 0.4109221d is also possible.
V0725 Lyr | VB A (B 16.7mpg, 6", 102deg, 2000).
V0730 Lyr | SRB type with P = 85d is also possible.
V0742 Lyr | Pulsations: P = 40d - 50d, amplitude 0.4m.
V0753 Lyr | VB A (B 4", 178deg, 1998).
V0754 Lyr | O'Connell effect.
V0755 Lyr | O'Connell effect.
V0757 Lyr | Periods 2.2148d or 2.8458d are also possible.
V0758 Lyr | O'Connell effect.
V0766 Lyr | O'Connell effect.
V0775 Lyr | O'Connell effect.
V0778 Lyr | RRC type with P = 0.29403d or P = 0.2270d is also possible.
V0780 Lyr | VB A (B 17.1m, 5", 307deg, 1998).
V0781 Lyr | VB A (B 17.3m, 6", 191deg, 1998). The one-day alias, P = 0.055562d, is also possible.
V0784 Lyr | O'Connell effect.
V0785 Lyr | Strong O'Connell effect.
V0798 Lyr | Not red.
V0817 Lyr | EW type with a twice longer period is not excluded.
DS    Mic | Period varies [81001].
V2970 Oph | Type EB with P = 0.749593d is not excluded.
V2975 Oph | VB (about 3"). Probably the eastern component is the variable.
V2976 Oph | Blazhko effect, P = 36d.
V2980 Oph | VB A (B 5", 120deg, 1998).
V2981 Oph | VB A (B 6", 23deg, 1998).
V3002 Oph | Blazhko effect, P = 28.58d.
V3003 Oph | Type EB with P = 0.713648d is not excluded.
V3014 Oph | Several close companions.
V3017 Oph | Several close companions.
V3068 Oph | RRC type with a twice shorter period is also possible.
V3072 Oph | RRC type with a twice shorter period is also possible.
V3079 Oph | VB B (AB 4", 206deg, 2000). The magnitudes in the Table were influenced by the companion.
V3095 Oph | A twice longer period is also possible.
V3099 Oph | VB A (B 3.5", 256 deg, 1999). The magnitudes in the Table were influenced by the companion.
V3128 Oph | VB A (B 7", 326deg, 2000).
V3138 Oph | A twice longer period is also possible.
V3141 Oph | Not red.
V3149 Oph | VB A (B 14.1m, 11", 338deg, 1991).
V3157 Oph | RRC type with a twice shorter period is also possible.
V3158 Oph | VB A (B 14.4mV, 6.5", 86deg, 2000).
V3169 Oph | RRC type with a twice shorter period is also possible.
V3181 Oph | DSCT type with a twice shorter period is also possible.
V3189 Oph | VB A (B 4", 188deg, 2000). The magnitudes in the Table were influenced by the companion.
V3201 Oph | RRC type with a twice shorter period is also possible.
V3203 Oph | A twice shorter period is also possible.
V3232 Oph | Type RRC and P = 0.219324d are also possible.
V3233 Oph | P = 0.357913d is also possible.
V3273 Oph | P = 0.330540d is also possible.
V3280 Oph | EW type with P = 0.842916d is also possible.
V3290 Oph | Other possible periods: 0.399278d and 0.285235d.
V3294 Oph | VB (3"). The south-eastern component varies. The magnitudes in the Table were influenced by the companion.
V3301 Oph | EW type with P = 0.578142d is also possible.
V3303 Oph | Type EA or EB with P = 1.10753d is also possible.
V3312 Oph | P = 0.2948d is also possible.
V3331 Oph | O'Connell effect.
V3339 Oph | EW type with P = 0.32572d is also possible.
V3368 Oph | The one-day alias, P = 0.052743d, is also possible.
V3380 Oph | The one-day alias, P = 0.49813d, is also possible.
V3409 Oph | A twice longer period is also possible.
V3410 Oph | P = 0.285971 is also possible.
V3415 Oph | Other possible periods: P = 0.309472d (RRC type) or P = 0.618943 (EW type).
V3416 Oph | Other possible periods: 0.285741d (RRC type), 0.400063d (RRC type), 0.444211d (EW type), 0.571481d (EW type).
V3424 Oph | EW type with P = 0.200466d is also possible.
V3430 Oph | RRC type with P = 0.301831d is also possible.
V3470 Oph | RRC type with a twice shorter period is also possible.
V3489 Oph | P = 0.323339d is also possible.
V3502 Oph | VB A (B 4", 143deg, 2000).
V3504 Oph | DSCT type with a twice shorter period is also possible.
V3532 Oph | A twice longer period is also possible.
V3533 Oph | A one-day alias, P = 0.397451d, is also possible.
V3534 Oph | RRAB type with a twice shorter period is also possible.
V3541 Oph | VB A (B 4", 268deg, 1999). The magnitudes in the Table were influenced with the companion.
V3569 Oph | VB A (B 3", 329deg, 1999).
V3577 Oph | A one-day alias, P = 0.378940d, is also possible.
V3579 Oph | RRC type with a twice shorter period is also possible.
V3583 Oph | A one-day alias, P = 0.081429d, is also possible.
V3609 Oph | Blazhko effect, P = 53.4d.
V3616 Oph | VB (companion 4", 293deg, 1999).
V3617 Oph | VB A (B 15.4m, 5.5", 20deg, 1999). RRC type with P = 0.21753d is also possible.
V3618 Oph | VB (companion 5", 139deg, 1999).
V3627 Oph | Close companions. The light curve shape varies. RRC type with P = 0.2746d is also possible.
V3632 Oph | Close VB.
V3637 Oph | VB A (B 5", 118deg, 1999).
V3638 Oph | O'Connell effect.
V3640 Oph | Close companions.
V3642 Oph | O'Connell effect.
V3650 Oph | Close VB.
V3652 Oph | VB A (B 5", 337deg, 2000; other companions).
V3653 Oph | Crowded.
V3655 Oph | O'Connell effect.
V3656 Oph | O'Connell effect.
V3657 Oph | VB B (AB 6", 352deg, 1999).
V0430 Pav | Type EW with P=0.444342d is not excluded.
V0449 Pav | Blazhko effect, P = 61.3d.
V0624 Peg | SB, Porb = 0.05865d. High proper motion.
V0627 Peg | A close southern companion of GSC 02197-00866. High proper motion.
V0643 Peg | Double-mode pulsation. P2 = 0.73025d.
V0648 Peg | Double-mode pulsation. P2 = 0.220793d.
V0674 Peg | P = 0.3632d is not excluded.
KV    Psc | Multiperiodic. P2 = 0.289120d. P2/P1 = 0.9779.
LL    Psc | Double-mode pulsation. The period in the Table is for the first overtone. P0 = 0.468938d. P1/P0 = 0.7434.
AO    PsA | Period varies?
V0404 Sge | The light curve shape, including the depth of minima, varies.
V0407 Sge | P = 0.086636d is also possible.
V5672 Sgr | VB A (B 5", 35deg, 2000). The magnitudes in the Table were influenced by the companion.
V5675 Sgr | P = 129d is superposed.
V5680 Sgr | VB A (B 14.5mV, 6", 148deg, 1996).
V5695 Sgr | MinII - MinI = 0.56P.
V5697 Sgr | MinII - MinI = 0.59P.
V5700 Sgr | VB A (B 3.5" f).
V5701 Sgr | Several close companions.
V5728 Sgr | VB A (B 2.5" f).
V5731 Sgr | VB A (B 2.5" p).
V5732 Sgr | VB B (A 2" np).
V5743 Sgr | Several close companions.
V5745 Sgr | VB A (B 2" np).
V5759 Sgr | SB, Porb = 671d.
V5760 Sgr | VB B (A 2.5" nf). Eclipses: 16.9m - 17.2m, MinII 17.1m. A brightening to 15.0m, of unclear nature, was observed on JD2453050 - 2453170.
V5779 Sgr | Main wave: amplitude about 1.2m; long wave: P = 1566d, amplitude about 3m.
V5815 Sgr | VB A (B 11.9, 8", 235deg, 2000).
V5824 Sgr | VB A (B 13.0m, 7", 69deg, 1999).
V5825 Sgr | VB A (B = V2790 Sgr, 13", 271deg, 1980; also other companions).
V5830 Sgr | The identification with V1615 Sgr [81002] is wrong.
V5833 Sgr | Multiperiodic. Other periods: 0.1345604d; 0.0821122d?
V5837 Sgr | Multiperiodic, 5 harmonics detected.
V5840 Sgr | SB2.
V5845 Sgr | Double-mode pulsations. P1 is given in the Table, P0 = 0.45389d. P1/P0 = 0.7416.
V5846 Sgr | VB A (9.53m; B 10.9m, 13", 106deg, 1999). The magnitudes in the Table are influenced with the companion.
V5847 Sgr | The elements in the Table are for the first overtone. P0 = 0.474648d. P1/P0 = 0.7439.
V1628 Sco | VB B (A 11.2m; AB 15", 220deg, 1999). The tabulated magnitude in maximum was influenced by component A.
V1644 Sco | VB A (B 5", 114deg, 1999).
V1646 Sco | VB A (B 12.2m, 17", 355deg, 1999).
V1653 Sco | VB B (A 12.6m; AB 9", 21deg, 1998). The magnitude at maximum in the Table is for the combined brightness.
V0509 Sct | Several close companions.
V0514 Sct | Several close companions.
V0521 Sct | VB B (A 13.7m; AB 4", 359deg, 1998).
V0530 Sct | VB B (A 3" sp).
V0531 Sct | VB (companion of comparable brightness, 4.5", 326deg, 1998).
V0548 Sct | Crowded.
V0556 Sct | Crowded.
V0558 Sct | Several companions.
V0567 Sct | Crowded.
V0571 Sct | Crowded.
V0573 Sct | Crowded.
V0574 Sct | Crowded.
V0575 Sct | Crowded.
V0584 Sct | Crowded.
V0600 Sct | VB A (B 2" nf).
V0609 Ser | VB A (B 4", 186deg, 1998; several fainter companions). The magnitudes in the Table were influenced by the companions.
V0627 Ser | A twice shorter period is also possible. VB A (B 7", 183deg; C 5", 159deg, 2000).
V0628 Ser | VB A (B 14.0mV, 7.5", 207deg, 2000).
V0384 Tel | VB A (B 6.5",40deg, 1999).
V0388 Tel | Double-mode pulsations. P0 is given in the Table, P1 = 0.1127701d. P1/P0 = 0.7564.
V0389 Tel | Blazhko effect, P = 10.82d.
EX    Tuc | SB2.
V0523 Vul | O'Connell effect. Unusually red for the EW type. VB B (A 14.6m; AB 4", 43deg, 1991).
V0524 Vul | P = 0.685447d and type EW are also possible.
V0528 Vul | P = 0.471026d is also possible.
V0532 Vul | VB A (B 8", 94deg, 2000; C 5", 247deg, 2000).
V0533 Vul | P = 0.267441d is also possible.
V0536 Vul | P = 0.269786d is also possible.
V0539 Vul | P = 0.3098d is also possible.
V0540 Vul | Other possible periods: 0.418246d or 0.294669d.
V0543 Vul | P = 0.274336d is also possible.
V0544 Vul | P = 1.60142d is also possible.