Light Curve of the Eccentric Eclipsing Binary GSC 3152-1202
Robert K. Buchheimn
Received February 25, 2011; accepted June 8, 2011
A complete light curve of this eccentric (~2.094d) eclipsing binary system has been determined, in B, V, and R bands. The primary and secondary minima are slightly different in depth, and the color index does not change during either primary or secondary eclipse. Newly-determined times of minimum confirm the previously-suspected rapid change in the orbital phase of the secondary minimum, implying significant apsidal motion.
Last Updated: December 6, 2011 - 5:32pm