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Dwarf Cepheid Variable Stars: A Study of CY Aquari

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Chris Dolan

Robin Tripoli

Jim Houck

Department of Astronomy, Cornell University, Ithaca, NY 14853

 

Received: June 11, 1993

 

Abstract

 

We report a period of 87.89534 +- 0.00015 minutes for the dwarf Cepheid variable star, CY Aquarii.  This result is based on observations made during September and October of 1992.  This value compares favorably to a published period of about 87.89517792 minutes.

 

Link to ADS abstract, article and citation information

 
 
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