Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901

Details Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901 Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901

2007-11-13

arxiv.org/abs/0711.1966v1

Astrophys.SpaceSci.313:419-423,2008

Astronomy and Astrophysics

Astrophysics

Accepted for publication in Astrophysics & Space Science

Scientific paper

10.1007/s10509-007-9711-5

Photometric analysis of $BVR_C$ light curves of newly discovered eclipsing binary GSC 0008-00901 is presented. The orbital period is improved to 0.28948(11) days. Photometric parameters are determined, as well. The analysis yielded to conclusion that system is an over-contact binary of W UMa type with components not in thermal contact. The light curves from 2005 show the presence of a spot on the surface of one of the components, while light curves from 2006 are not affected by maculation.

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