The evolution of intermediate mass close binary systems: scenarios leading to novae

Details The evolution of intermediate mass close binary systems: scenarios leading to novae The evolution of intermediate mass close binary systems: scenarios leading to novae

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637...62g&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 6

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Astrometric And Interferometric Binaries, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Cataclysmic Binaries, Symbiotic Stars, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We revisit the problem of the determination of the frequency of occurrence of ONe white dwarfs in galactic novae. In doing that we use our evolutionary scenarios for intermediate mass close binary systems. We also consider observational selection effects. Our results indicate that approximately 1/3 of the observed novae should host an ONe white dwarf.

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