Photometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901

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dc.creatorParimucha, S.
dc.creatorPribulla, T.
dc.creatorVaňko, M.
dc.creatorDubovsky, P.
dc.creatorHambalek, L.
dc.date2007-11-13
dc.date.accessioned2026-07-07T11:13:08Z
dc.date.available2026-07-07T11:13:08Z
dc.descriptionPhotometric 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.
dc.descriptionAccepted for publication in Astrophysics & Space Science
dc.identifierhttps://arxiv.org/abs/0711.1966
dc.identifierhttp://arxiv.org/abs/0711.1966
dc.identifierAstrophys.SpaceSci.313:419-423,2008
dc.identifierdoi:10.1007/s10509-007-9711-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191613
dc.subjectAstrophysics
dc.titlePhotometric Analysis of Recently Discovered Eclipsing Binary GSC 00008-00901
dc.typetext

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