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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2763
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dc.contributor.authorRukmini, J-
dc.contributor.authorRao, P. V-
dc.date.accessioned2008-07-21T09:59:14Z-
dc.date.available2008-07-21T09:59:14Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 665 - 670en
dc.identifier.urihttp://hdl.handle.net/2248/2763-
dc.description.abstractStudy 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.extent134532 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectPhotometric Studyen
dc.subjectOpen Cluster Be 33en
dc.subjectWilson-Devinney Methoden
dc.titlePhotometric study of two W UMa-type systems in the intermediate age open cluster Be 33en
dc.typeArticleen
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