Thermonuclear Runaway Models for Symbiotic Novae
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)
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.
KeywordsAccretion 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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