V0769 And VB B (A 16.8mV, B 16.9mV; AB 6", 37deg, 1998). The magnitudes in the
V0769 And  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.
V0367 Aqr  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:
V0370 Aqr  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
V0371 Aqr  mode. P1=0.0624379d. P1/P0=0.7748.
V0373 Aqr Double-mode pulsation. The period in the Table is for the first
V0373 Aqr  overtone. P0=0.554570d. P1/P0=0.7456.
V0375 Aqr Double-mode pulsation. The period in the Table is for the first
V0375 Aqr  overtone. P0=0.479278d. P1/P0=0.7443.
V0379 Aqr Double-mode pulsation. The period in the Table is for the first
V0379 Aqr D overtone. P0=0.395471d. P1/P0=0.7459.
V0380 Aqr Double-mode pulsation. The period in the Table is for the first
V0380 Aqr  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.
V1837 Aql  Second overtone: Max=2453729.40+ 1.01121d x E. P1 given in the
V1837 Aql  Table. P2/P1=0.8040.
V1844 Aql Multiperiodic.
V1853 Aql VB (2"). Other possible periods: 0.66579d or 0.49934d.
V1853 Aql  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
V1027 Ara  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.
VY    Equ  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
V1446 Her  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.
V0524 Lac  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,
V0781 Lyr  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
V3079 Oph  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
V3099 Oph  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
V3189 Oph  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
V3294 Oph  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),
V3416 Oph  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
V3541 Oph  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).
V3617 Oph  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.
V3627 Oph  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
LL    Psc  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
V5672 Sgr  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
V5760 Sgr  to 15.0m, of unclear nature, was observed on JD2453050 - 2453170.
V5779 Sgr Main wave: amplitude about 1.2m; long wave: P=1566d,
V5779 Sgr  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.
V5845 Sgr  P1/P0=0.7416.
V5846 Sgr VB A (9.53m; B 10.9m, 13", 106deg, 1999). The magnitudes in the Table
V5846 Sgr  are influenced with the companion.
V5847 Sgr The elements in the Table are for the first overtone. P0=0.474648d.
V5847 Sgr  P1/P0=0.7439.
V1628 Sco VB B (A 11.2m; AB 15", 220deg, 1999). The tabulated magnitude in
V1628 Sco  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
V1653 Sco  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
V0609 Ser  in the Table were influenced by the companions.
V0627 Ser A twice shorter period is also possible.
V0627 Ser  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.
V0388 Tel D 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.
V0523 Vul  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.