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.
