Light Curve Analysis of SAO23229

Details Light Curve Analysis of SAO23229 Light Curve Analysis of SAO23229

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jass...10...36k&link_type=abstract

Journal of Astronomy and Space Sciences, vol.10, no 1, p.36-43.

Astronomy and Astrophysics

Astronomy

Scientific paper

We have made UBV light curves of a newly discovered eclipsing binary, SAO23229 at Sobaeksan Astronomy Observatory. We determined a minimum light time of HJD2448636.1170+/-0.0005 that is 3 minutes later than predicted time, and founda peculiar light variation at phase 0.75 that may not be secondary eclipse. Orbital period of SAO23229 would be 4.2 days rather than 2.1 days. Our analysis of the light curves shows that SAO23229 has a detached configuration consisting of two almost identical F type main sequence stars.

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