Period-mass ratio relations for eclipsing binaries with periods not exceeding 5 days

dc.contributor.author	Sinvhal, S. D.
dc.contributor.author	Srivastava, J. B.
dc.date.accessioned	2011-11-14T05:34:46Z
dc.date.available	2011-11-14T05:34:46Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/865
dc.description.abstract	The dependence of mass ration of eclipsing binary system on period has been studied. It has been found that semi-detached systems obey the relation m₂/m₁ = 0.64 - 0.079P or m₂/m₁ = 0.29 - 0.028P depending upon whether the mass ratio is >0.3 or <0.3. The mass ratio of detached systems generally appears to be independent of the period.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass54-239
dc.subject	Eclipsing Binaries	en_US
dc.title	Period-mass ratio relations for eclipsing binaries with periods not exceeding 5 days	en_US
dc.type	Article	en_US