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Thermonuclear Runaway Models for Symbiotic Novae

  • Scott J. Kenyon
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)

Abstract

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.

Keywords

Accretion Rate White Dwarf Mass Accretion Rate Bolometric Luminosity Symbiotic Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • Scott J. Kenyon
    • 1
  1. 1.Smithsonian Astrophysical ObservatoryHarvard-Smithsonian Center for AstrophysicsCambridgeUSA

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