Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901

S. Parimucha; T. Pribulla; M. Vaňko; P. Dubovsky; L. Hambalek

doi:10.1007/s10509-007-9711-5

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arXiv · 0711.1966

Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901

S. Parimucha·T. Pribulla·M. Vaňko·P. Dubovsky·L. Hambalek

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Abstract

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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S. Parimucha, T. Pribulla, M. Vaňko, P. Dubovsky, L. Hambalek. 2007-11-13. Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901. https://doi.org/10.1007/s10509-007-9711-5

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