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http://hdl.handle.net/2248/4495
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DC Field | Value | Language |
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dc.contributor.author | Anupama, G. C | - |
dc.date.accessioned | 2009-05-26T13:57:29Z | - |
dc.date.available | 2009-05-26T13:57:29Z | - |
dc.date.issued | 1995 | - |
dc.identifier.citation | A. Bianchini, M. della Valle, and M. Orio., ed., Cataclysmic Variables, Proceedings of the conference held in Abano Terme, Italy, 20 - 24 June, 1994, pp. 49 - 57 | en |
dc.identifier.isbn | 0-7923-3676-3 | - |
dc.identifier.uri | http://hdl.handle.net/2248/4495 | - |
dc.description | Restricted Access | - |
dc.description.abstract | The observational properties of recurrent novae are reviewed in this talk. The class of recurrent novea may be divided into subgroups as (a) systems with a dwarf secondary and (b) systems with a giant secondary. The primary in these systems is a white draf, accreting at rates ~ 18/sup-8 M yr/sup-1. The outbursts are poweres by thermonuclear runaway reactions on the surface of the white dwarf. | en |
dc.language.iso | en | en |
dc.publisher | Kluwer Academic Publishers | en |
dc.relation.ispartofseries | Astrophysics and Space Science Library; Vol. 205 | - |
dc.subject | Recurrent Novae | en |
dc.title | The general trends of recurrent novae | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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The general trends of recurrent novae Restricted Access | Restricted Access | 4.8 MB | Adobe PDF | View/Open Request a copy |
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