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http://hdl.handle.net/2248/4495| Title: | The general trends of recurrent novae |
| Authors: | Anupama, G. C |
| Keywords: | Recurrent Novae |
| Issue Date: | 1995 |
| Publisher: | Kluwer Academic Publishers |
| 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 |
| Series/Report no.: | Astrophysics and Space Science Library; Vol. 205 |
| 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. |
| Description: | Restricted Access |
| URI: | http://hdl.handle.net/2248/4495 |
| ISBN: | 0-7923-3676-3 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| The general trends of recurrent novae Restricted Access | Restricted Access | 4.8 MB | Adobe PDF | View/Open Request a copy |
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