Binary system parameters and the hibernation model of cataclysmic variables

Details Binary system parameters and the hibernation model of cataclysmic variables Binary system parameters and the hibernation model of cataclysmic variables

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...319..819l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 319, Aug. 15, 1987, p. 819-826.

Astronomy and Astrophysics

Astrophysics

28

Binary Stars, Cataclysmic Variables, Mass Transfer, Novae, Stellar Evolution, Stellar Models, Dwarf Novae, Statistical Analysis

Scientific paper

The "hibernation" model, in which nova systems spend most of the time between eruptions in a state of low mass transfer rate, is examined. The authors determine which binary systems are more likely to undergo hibernation. The predictions of the hibernation scenario are shown to be consistent with available observational data. The authors indicate how the hibernation scenario provides links between classical novae, dwarf novae, and novalike variables, all of which represent different stages in the cyclic evolution of the same systems.

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