Light Curve of the of Eccentric Eclipsing Binary GSC 3152-1202

Details Light Curve of the of Eccentric Eclipsing Binary GSC 3152-1202 Light Curve of the of Eccentric Eclipsing Binary GSC 3152-1202

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011javso..39..170b&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 39, nr. 2, p. 170

Computer Science

Scientific paper

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.

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