Photometric study of eclipsing binaries in the Large Magellanic Cloud — I. W UMa type binaries in the Large Magellanic Cloud
Abstract
Eclipsing binaries are among the most important sources of information on stellar parameters like radii, masses, luminosities, etc. We present the analysis of six W UMa systems discovered in the Large Magellanic Cloud using the Wilson-Devinney method.
- Publication:
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Research in Astronomy and Astrophysics
- Pub Date:
- February 2011
- DOI:
- Bibcode:
- 2011RAA....11..175S