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

dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2010-01-27T06:45:21Z
dc.date.available	2010-01-27T06:45:21Z
dc.date.issued	1990
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/474
dc.description.abstract	Twenty-seven typical binary systems have been investigated to study their power-output by gravitational radiation (Pв) and spiralling time (τₒ) relation. It was found that these binary systems form two distinct groups. New relations have been given between Pв and τₒ for each group.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass167-161
dc.subject	Closed binary systems, Gravitational radiation (Pв), Spiralling time (τₒ)	en_US
dc.title	Gravitational radiation and spiralling time of close binary systems (III)	en_US
dc.type	Article	en_US