The general trends of recurrent novae

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