Classical novae crossing the thermal stability line. I.

Details Classical novae crossing the thermal stability line. I. Classical novae crossing the thermal stability line. I.

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stast..36..250r&link_type=abstract

Astronomer, Vol. 36, No. 430, p. 250 - 254

Other

Novae: Stellar Evolution

Scientific paper

A general review of the transitions in non-magnetic novae, and their evolutionary connections with other subclasses of cataclysmic variables (CVs) is discussed. New evolutionary scenarios are suggested for short orbital period CVs. The presence of a new type of nova, a helium nova, is also speculated based on the suggestion to extend the scenarios to the AM CVn systems.

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