Precise Distances to the Magellanic Clouds From Unique Late-Type Long-Period Eclipsing Binaries

Details Precise Distances to the Magellanic Clouds From Unique Late-Type Long-Period Eclipsing Binaries Precise Distances to the Magellanic Clouds From Unique Late-Type Long-Period Eclipsing Binaries

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..435...13p&link_type=abstract

Binaries - Key to Comprehension of the Universe. Proceedings of a conference held June 8-12, 2009 in Brno, Czech Republic. Edite

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We will present first results on distance determination to the LMC and SMC based on very rare late-type long-period eclipsing binaries with G-type giant components. It has been demonstrated that using accurate photometric and spectroscopic data and well established surface-brightness color (V-K) relations one can measure distances to individual systems with an accuracy of 3 per cent. With the discovery of a few dozen such systems in the Magellanic Clouds we are in a position to be able to measure distances to the LMC and SMC with 1 and 2.

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