The Lightcurve of UZ Sge

Details The Lightcurve of UZ Sge The Lightcurve of UZ Sge

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sass...28..181b&link_type=abstract

The Society for Astronomical Sciences 28th Annual Symposium on Telescope Science. Held May 19-21, 2009 at Big Bear Lake, CA. Pub

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Scientific paper

A complete lightcurve of the eclipsing binary UZ Sge has been determined, in V- and R-bands. Four new times of minimum are reported (two for primary eclipse and two for secondary eclipse), which verify other recent O-C observations. The color index changes significantly during both primary eclipse and secondary eclipse, providing some constraints on the stars' temperatures. BinaryMaker3 software has been used to compare the observed V- and R- lightcurves with two models of this system (with quite different mass ratios of q= 0.14 and q= 0.68, respectively) that have been suggested in the literature.

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