Gravitational radiation and spiralling time of close binary systems (II)

dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2010-02-16T06:29:59Z
dc.date.available	2010-02-16T06:29:59Z
dc.date.issued	1988
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/524
dc.description.abstract	Power-output by gravitational radiation (Pв) and spiralling time (τₒ) for individual systems of twelve early (B) type binary systems have been evaluated. A new relation between Pв and τₒ obtained. It is found that most of these systems lie in the spiralling time range ~10⁹ years.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass149-379
dc.subject	Close binary systems (II)	en_US
dc.title	Gravitational radiation and spiralling time of close binary systems (II)	en_US
dc.type	Article	en_US