Period study of the RS CVn eclipsing binary SV Camelopardalis

Sarma, C. V. S. R. ; Sarma, M. B. K. ; Abhyankar, K. D. (1985) Period study of the RS CVn eclipsing binary SV Camelopardalis Bulletin of the Astronomical Society of India, 13 . pp. 346-358. ISSN 0304-9523

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Official URL: http://adsabs.harvard.edu/abs/1985BASI...13..346S

Abstract

Using the available photographic and photoelectric times of minima, we have revised the elements of the light-time orbit of SV Camelopardalis, an RS CVn type eclipsing binary. Taking a mass function of 0.118 M and the inclination of 89°.84 for the eclipsing pair, we obtain the third body mass of 0.18, 0.21 and 0.38 M for the assumed inclination of the third body orbit of 90° , 60° and 30° respectively.

Item Type:Article
Source:Copyright of this article belongs to Astronomical Society of India.
Keywords:Eclipsing Binary; RS CVn Binaries; SV Cam; Triple System
ID Code:24041
Deposited On:01 Dec 2010 12:42
Last Modified:17 May 2016 07:49

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