Changes in the binary system parameters resulting from nova explosions

Details Changes in the binary system parameters resulting from nova explosions Changes in the binary system parameters resulting from nova explosions

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...246...84l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 246, no. 1, June 1991, p. 84-90. Research supported by S. Faust Research Fund

Astronomy and Astrophysics

Astrophysics

26

Cataclysmic Variables, Novae, Stellar Evolution, Stellar Orbits, Angular Momentum, White Dwarf Stars

Scientific paper

The effect of nova outbursts on the binary separation is examined. It is
found that as a result of strong nova explosions, the orbital period of
short period systems decreases, while the orbital period of long period
systems increases. Some observational consequences and the effects of
the separation changes on models of secular evolution are discussed.

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