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Edward Schmidt Publications
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Document Type
Article
Date of this Version
November 1989
Abstract
The relationships between the periods and the rate of decline in V and R for pulsating stars are investigated. It is shown that these relationships are useful for making preliminary estimates of periods for stars with little data. These estimates can then be used to optimize times of further observations.
Comments
Published in The Astronomical Journal 98, 1659 (1989). Published by the University of Chicago Press; copyright © 1989 American Astronomical Society; reproduced by permission of the AAS. http://www.journals.uchicago.edu/AJ/