Period study of the RS CVn eclipsing binary SV Camelopardalis

dc.contributor.author	Sarma, C. V. S. R
dc.contributor.author	Sarma, M. B. K
dc.contributor.author	Abhyankar, K. D
dc.date.accessioned	2005-12-08T04:55:17Z
dc.date.available	2005-12-08T04:55:17Z
dc.date.issued	1985-12
dc.identifier.citation	BASI, Vol. 13, No. 4, pp. 346-358	en
dc.identifier.uri	http://hdl.handle.net/2248/665
dc.description.abstract	Using 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.extent	898771 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Eclipsing binary	en
dc.subject	RS CVn binaries	en
dc.subject	SV Cam	en
dc.subject	Triple system	en
dc.title	Period study of the RS CVn eclipsing binary SV Camelopardalis	en
dc.type	Article	en