2002PASP..114..546L

Query : 2002PASP..114..546L

2002PASP..114..546L - Publ. Astron. Soc. Pac., 114, 546-550 (2002/May-0)

The Blazhko effect of the RR Lyrae star GV Andromedae.

LEE K.M., SCHMIDT E.G. and LANGAN S.T.

Abstract (from CDS):

We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is consistent with a primary period of 0.528092 days; however, the light curve of GV And cannot be well described by a single period. We conclude that GV And demonstrates the Blazhko effect with a Blazhko period of approximately 32 days.

Abstract Copyright: ∼

Journal keyword(s): stars: individual (GV Andromedae) - Stars: Variables: Other

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* DR And RR* 01 05 10.7138848320 +34 13 06.289699800   13.66 12.42     ~ 71 1
2 V* FM Per RR* 04 03 27.0822047952 +47 59 51.840080052     12.70     ~ 27 0
3 V* RV UMa RR* 13 33 18.0838837128 +53 59 14.598026988   10.97 10.9     kA9hF7 182 0
4 V* V442 Her RR* 18 12 58.4336412312 +42 03 45.948939840     13.25     ~ 29 0
5 V* GV And RR* 23 13 12.5459809512 +36 54 04.361142636   13.0 14.04     ~ 24 0
6 GSC 02763-00475 * 23 13 22.6964128608 +36 53 04.920466380           ~ 1 0

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