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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/665
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dc.contributor.authorSarma, C. V. S. R-
dc.contributor.authorSarma, M. B. K-
dc.contributor.authorAbhyankar, K. D-
dc.date.accessioned2005-12-08T04:55:17Z-
dc.date.available2005-12-08T04:55:17Z-
dc.date.issued1985-12-
dc.identifier.citationBASI, Vol. 13, No. 4, pp. 346-358en
dc.identifier.urihttp://hdl.handle.net/2248/665-
dc.description.abstractUsing the available photographic and photoelectric times of minima, we have revised the elements of the light-time orbit of SV Camelopaedalis, an RS CVn type eclpsing binary. Taking a mass function of 0.118 M and the inclination of 89/sup0/.84 and 0.38 M for the assumed inclination of the third body orbit of 90/supo/, 60/sup0/ and 30/sup0/ respectively.en
dc.format.extent898771 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectEclipsing binaryen
dc.subjectRS CVn binariesen
dc.subjectSV Camen
dc.subjectTriple systemen
dc.titlePeriod study of the RS CVn eclipsing binary SV Camelopardalisen
dc.typeArticleen
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