Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud

Details Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud Light Curve Analyses of the Eclipsing Binary EROS 1010 in the Large Magellanic Cloud

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jass...26..295h&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 26, no. 3, 295-304

Astronomy and Astrophysics

Astronomy

Eclipsing Binaries, Lmc, Data Analysis

Scientific paper

We present BV light curves of EROS 1010 which is located in the central bar of the Large Magellanic Cloud. The BV light curves including BR and I light curves observed by the EROS and OGLE projects, have been analyzed using the 2005 version of the Wilson & Devinney Differential Correction program for the photometric solutions. The absolute dimensions of EROS 1010 were calculated by adopting the distance modulus of the Large Magellanic Cloud, m-M = 18.m3 ~ 18.m5.

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