Evolutionary processes in close binary stars

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2010-03-10T07:08:08Z
dc.date.available	2010-03-10T07:08:08Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/632
dc.description.abstract	The evolutionary processes of close binary stars have been examined. It is found that there is a strong deficit of binaries evolving in Case A in the whole mass range. Probably the binary stars having binary separation corresponding to Case A evolution form.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass103-385
dc.subject	Close binary stars	en_US
dc.title	Evolutionary processes in close binary stars	en_US
dc.type	Article	en_US