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V714 Cygni: A Study in the Evolution of a RL Herculis Star

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Clay Holroyd

Maria Mitchell Observatory, Nantucket, MA 02554

 

Received: 5 January 1990

 

Abstract

 

An increasing period determined for V714 Cygni suggests evolutionary changes. A comparison with quantities derived from evolutionary models indicates a possible helium abundance and mass.

 

Link to ADS abstract, article and citation information

 
 
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