The evolution of a slow nova model with a Z = 0.03 envelope from pre-explosion to extinction

Details The evolution of a slow nova model with a Z = 0.03 envelope from pre-explosion to extinction The evolution of a slow nova model with a Z = 0.03 envelope from pre-explosion to extinction

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62..339p&link_type=abstract

Astronomy and Astrophysics, vol. 62, no. 3, Jan. 1978, p. 339-348.

Astronomy and Astrophysics

Astrophysics

85

Novae, Stellar Envelopes, Stellar Evolution, Stellar Mass Ejection, Stellar Models, Abundance, Stellar Luminosity, Stellar Temperature, Thermonuclear Reactions, Time Dependence, White Dwarf Stars

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1978A&A....62..339P

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