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

dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2010-01-13T10:46:10Z
dc.date.available	2010-01-13T10:46:10Z
dc.date.issued	1992
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/424
dc.description.abstract	Forty-six binary systems with their primary component masses between 2 M☉ and M☉ have been considered for gravitational radiation study. Power output by gravitational radiation (Pв) and spiral τ0 for all individual systems have been evaluated. A relation has been given between Pв and τ0. The rate of decrease of orbital period (Ṗ) has also been given for 10 eccentric orbit systems.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass202-63
dc.subject	Binary systems, Gravitational radiations	en_US
dc.title	Gravitational radiation and spiralling time of close binary systems (V)	en_US
dc.type	Article	en_US