Eclipsing binary UW Bootis

dc.contributor.author	Srivastava, J. B.
dc.contributor.author	Kandpal, C. D.
dc.date.accessioned	2010-02-24T05:17:30Z
dc.date.available	2010-02-24T05:17:30Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/572
dc.description.abstract	Photometric observations of primary minimum in U, B, and V filters have been discussed. The amplitude of variation in all three filter is 0.ͫ66. We do not find variations in the period and its revised value is 0.ͩ0047115.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass133-291
dc.subject	Eclipsing binary system UW Bootis	en_US
dc.title	Eclipsing binary UW Bootis	en_US
dc.type	Article	en_US