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Evolution of a Degenerate Component in a Close Binary System

Published online by Cambridge University Press:  12 April 2016

E.V. Ergma
E.V. Ergma*
Affiliation:
Astronomical Council, USSR Academy of Sciences

Extract

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Investigation of evolution of a degenerate component (helium or carbon-oxygen dwarf) in a close binary system is rather important. Such dwarfs may be candidates for nova or supernova stars. The first possibility has been studied by several authors (see review paper by Starrfield et al., 1976) and it has been shown that explosive hydrogen burning with enriched CNO abundance in the degenerate envelope of a massive carbon-oxygen dwarf may explain nova phenomena.

Type
Colloquium Session I
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 48 - 51
Copyright
Copyright © The University of Rochester 1979

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