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Edward Schmidt Publications
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Document Type
Article
Date of this Version
July 2001
Abstract
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identified a primary period of 0.489256 days; however, the light curve of FM Per cannot be well described by a single period. We conclude that FM Per demonstrates the Blazhko effect with a Blazhko period of approximately 122 days.
Comments
Published by the University of Chicago Press. The Astronomical Journal. Copyright 2001 American Astronomical Society. Reproduced by permission of the AAS. Permission to use. PASP 113, 835 (2001). http://www.journals.uchicago.edu/PASP/.