Light Curve Analysis of Early-Type Close Lmc Binaries

Details Light Curve Analysis of Early-Type Close Lmc Binaries Light Curve Analysis of Early-Type Close Lmc Binaries

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.296..235n&link_type=abstract

Astrophysics and Space Science, Volume 296, Issue 1-4, pp. 235-238

Astronomy and Astrophysics

Astrophysics

Binaries, Light Curves, Lmc, Ob-Type Stars

Scientific paper

Results are presented of an analysis of eclipsing binaries in the Large Magellanic Cloud. The sample of close OB-type stars was taken from the MACHO microlensing survey. The present study was restricted to systems with orbital periods shorter than 2 days and V and R light curves with large eclipse amplitudes, high S/N and homogeneous and dense phase coverage. Problems encountered during the analysis are discussed, especially with respect to the degeneracy of photometric mass ratios and other parameter correlations.

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