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Thermonuclear Runaway Models for Symbiotic Novae

Published online by Cambridge University Press:  12 April 2016

Scott J. Kenyon
Scott J. Kenyon*
Affiliation:
Smithsonian Astrophysical Observatory Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138, USA

Abstract

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This paper reviews the basic physics of thermonuclear runaways on the surfaces of accreting white dwarf stars, with a special emphasis on understanding the evolution of symbiotic novae.

Type
Session 2. The Physics of the Symbiotic Phenomenon
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 161 - 168
Copyright
Copyright © Kluwer 1988

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