Period study of the RS CVn eclipsing binary SV Camelopardalis

Details Period study of the RS CVn eclipsing binary SV Camelopardalis Period study of the RS CVn eclipsing binary SV Camelopardalis

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..346s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, Dec. 1985, p. 346-358. Research supported by the Indian Space Research Organiz

Astronomy and Astrophysics

Astronomy

6

Astrometry, Eclipsing Binary Stars, Stellar Orbits, Light Curve, Orbital Elements, Stellar Mass

Scientific paper

Using the available photographic and photoelectric times of minima, the authors 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_sun; and the inclination of 89°.84 for the eclipsing pair, the authors obtain the third body mass of 0.18, 0.21 and 0.38 M_sun; for the assumed inclination of the third body orbit of 90°, 60° and 30° respectively.

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