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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2274
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dc.contributor.authorRukmini, J-
dc.contributor.authorVivekananda Rao, P-
dc.contributor.authorAusekar, B. D-
dc.date.accessioned2008-05-08T09:40:05Z-
dc.date.available2008-05-08T09:40:05Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 323 - 327en
dc.identifier.urihttp://hdl.handle.net/2248/2274-
dc.description.abstractPhotoelectric B, V observations of the eclipsing binary system FZ Orionis obtained from the Japal-Rangapur Observatory during the years 1981 to 1992 are presented and studied. No period changes in the system are detected. The light curves are analysed using the Wilson-Devinney method and the system parameters are derived.en
dc.format.extent355475 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..323Ren
dc.subjectPhotoelectricen
dc.subjectW UMa systemen
dc.subjectFZ Orionisen
dc.titlePhotometric study of the short period W UMa system - FZ Orionisen
dc.typeArticleen
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