Gravitational radiation and spiralling time of close binary system

dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2010-02-19T05:16:32Z
dc.date.available	2010-02-19T05:16:32Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/552
dc.description.abstract	Power-output be gravitational radiation (Pв)and spiral time (τₒ) for individual systems of sixteen eclipsing binary stars have been evaluated, and a relation between Pв and τₒ obtained.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass137-191
dc.subject	Close binary system	en_US
dc.title	Gravitational radiation and spiralling time of close binary system	en_US
dc.type	Article	en_US