The role of thermonuclear instability in recent models of novae

Details The role of thermonuclear instability in recent models of novae The role of thermonuclear instability in recent models of novae

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ncimb..65..345s&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 65 B, Oct. 11, 1981, p. 345-403. In Italian. Research supported by the Consiglio Nazionale dell

Physics

Novae, Stellar Models, Thermonuclear Reactions, Degenerate Matter, Dynamic Models, Electron Gas, Ideal Gas, Radiation Pressure, Stellar Envelopes, Stellar Evolution, Stellar Structure, Stellar Temperature, Supernova Remnants

Scientific paper

The most salient results of theoretical models of nova explosions are
summarized, and the many problems that are still unresolved are
discussed. In particular, thermonuclear instabilities, thought to lie at
the base of the nova explosion phenomenon, are analyzed both for perfect
gas and degenerate electron gas.

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