Colour excess of eclipsing binaries in the Small Magellanic Cloud

Details Colour excess of eclipsing binaries in the Small Magellanic Cloud Colour excess of eclipsing binaries in the Small Magellanic Cloud

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..273n&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We give an estimate of the colour excess of eclipsing binaries in the Small Magellanic Clouds, estimated on the basis of OGLE (B-V) indices and interpolation in theoretical evolutionary tracks for Z=0.004, assuming equal components and a known distance modulus of 18.9. We also give the physical parameters of the average component for each binary, and compare them with results obtained by Graczyk (2003).

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