Photometric study of two W UMa-type systems in the intermediate age open cluster Be 33

dc.contributor.author	Rukmini, J
dc.contributor.author	Rao, P. V
dc.date.accessioned	2008-07-21T09:59:14Z
dc.date.available	2008-07-21T09:59:14Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 665 - 670	en
dc.identifier.uri	http://hdl.handle.net/2248/2763
dc.description.abstract	Study of eclipsing binaries in open clusters offers information regarding the age of the cluster in addition to the properties of the component stars. In this paper we present the analysis of two W UMa systems discovered in the open cluster Be 33 using the Wilson - Devinney method.	en
dc.format.extent	134532 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Photometric Study	en
dc.subject	Open Cluster Be 33	en
dc.subject	Wilson-Devinney Method	en
dc.title	Photometric study of two W UMa-type systems in the intermediate age open cluster Be 33	en
dc.type	Article	en