Light Curve Analyses of the Eclipsing Binaries in the Small Magellan Cloud

Details Light Curve Analyses of the Eclipsing Binaries in the Small Magellan Cloud Light Curve Analyses of the Eclipsing Binaries in the Small Magellan Cloud

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jass...25...77k&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 25, no. 2, 077-086

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binaries, Smc, Data Analysis

Scientific paper

Large survey observations such as the EROS, the MACHO and the OGLE projects have discovered a large number of eclipsing binaries in the extra galaxies and published their light curves. The light curves of the eclipsing binaries provide fundamental stellar parameters so that accumulation of the light curves will be very useful for the research of the stellar astronomy. However it requires a lot of time to analyze the light curves. Therefore we developed new method to analyze the large number of light curves in the relatively short time period and found the photometric solution by analyzing the light curves of 20 eclipsing binaries, whose mass ratio can be determined by photometic method, in the Small Magellan Cloud.

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