V714 Cygni: A Study in
the Evolution of a RL Herculis Star
Maria Mitchell Observatory,
Nantucket, MA 02554
Received: 5 January 1990
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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