Light Curve Solutions of Eclipsing Binaries in the Small Magellanic Cloud. II.
Abstract
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.
- Publication:
-
Publications de l'Observatoire Astronomique de Beograd
- Pub Date:
- September 2010
- Bibcode:
- 2010POBeo..90..137I