V714 Cygni: A Study in the Evolution of a BL Herculis Star
Volume 18 number 2 (1989)
- Clay Holroyd
- Maria Mitchell Observatory,
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. NOTE: The author of this article has posted an erratum by E. Belserene: https://app.aavso.org/jaavso/article/1253/