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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

L. Luud
L. Luud*
Affiliation:
Institute of Astrophysics & Atmospheric Physics, 202444 Tartu, Estonia, U.S.S.R.

Extract

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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

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