BVR photometry of a newly identified RS CVn binary star HD 61396

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dc.contributor.authorBarway, Sudhanshu
dc.contributor.authorPandey, S. K.
dc.date.accessioned2012-03-07T05:25:47Z
dc.date.available2012-03-07T05:25:47Z
dc.date.issued2011-07-06
dc.description.abstractBVR photometry of a recently identified RS CVn binary star HD 61396, carried out during 2001, is presented. The new photometry reveal significant evolution in the shape and amplitude of light curve when compared with those reported earlier by Padmakar et al.(2000). The traditional two-starspot model has been used to obtain the spot parameters from the observed light curve. Changes in the spot area and their location on the stellar surface are discernible from the extracted parameters from the new photometry.en_US
dc.identifier.urihttp://hdl.handle.net/11007/797
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;24/04
dc.subjectStar:activityen_US
dc.subjectStar:spotsen_US
dc.subjectStar:individual:HD 61396en_US
dc.subjectStars:lateen_US
dc.titleBVR photometry of a newly identified RS CVn binary star HD 61396en_US
dc.typeArticleen_US

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