New evolutionary scenarios for short orbital period CVs

Details New evolutionary scenarios for short orbital period CVs New evolutionary scenarios for short orbital period CVs

1999-05-28

arxiv.org/abs/astro-ph/9905378v1

Astronomy and Astrophysics

Astrophysics

2 pages, Latex file, 1 .sty file, to appear in "Cataclysmic Variables: a 60th Birthday Symposium in Honour of Brian Warner", h

Scientific paper

We suggest new evolutionary scenarios for non-magnetic short orbital period CVs. The first model is the analogy of the `hibernation scenario' or the `modern hibernation scenario'. The second one is an extension of Mukai and Naylor (1995) ideas. All models imply a tight connection between permanent superhump systems and classical novae. We highlight the significance of the observed evolution of V1974 Cyg, which might pose a major problem to Mukai and Naylor concept.

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