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CH Cygni – A White Dwarf and M-Giant Binary with Transient Accretion Disk
Published online by Cambridge University Press: 12 April 2016
Extract
The unusual variable star CH Cygni was an object of numerous investigations over past ten years. The aim of the present paper is to give a summary of the most important observational data and to discuss briefly a double star model of CH Cygni which is in general accordance with observational facts.
- Type
- Colloquium Session VII
- Information
- International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 459 - 463
- Copyright
- Copyright © The University of Rochester 1979