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Edward Schmidt Publications
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Document Type
Article
Date of this Version
May 2002
Abstract
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.
Comments
Published by the University of Chicago Press. The Astronomical Journal. Copyright 2002 American Astronomical Society. Reproduced by permission of the AAS. Permission to use. PASP 114, 546 (2002). http://www.journals.uchicago.edu/PASP/.