Light Curve Solutions of Eclipsing Binaries in the Small Magellanic Cloud. II.

Details Light Curve Solutions of Eclipsing Binaries in the Small Magellanic Cloud. II. Light Curve Solutions of Eclipsing Binaries in the Small Magellanic Cloud. II.

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..90..137i&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 90, pp. 137-140

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results from modeling of the light curves of 50 eclipsing
stars in the Small Magellanic Cloud (SMC) obtained in the framework of
the project OGLE. We established that the components of the target
binaries were hot stars with big relative radii and low densities.

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