New evolutionary scenarios for short orbital period CVs
| dc.creator | Retter, A. | |
| dc.creator | Naylor, T. | |
| dc.date | 1999-05-28 | |
| dc.date.accessioned | 2026-07-25T21:09:05Z | |
| dc.description | 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. | |
| dc.description | 2 pages, Latex file, 1 .sty file, to appear in "Cataclysmic Variables: a 60th Birthday Symposium in Honour of Brian Warner", held in Oxforf, 12-16/4/99, eds. P. Charles, A. King, D. O'Donoghue, New Astronomy Reviews. also available at: ftp://ftp.astro.keele.ac.uk/pub/preprints/Oxford.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9905378 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9905378 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/76707 | |
| dc.subject | Astrophysics | |
| dc.title | New evolutionary scenarios for short orbital period CVs | |
| dc.type | text |