Photometric and spectroscopic study of the eclipsing binary GSC 4288 0186

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dc.authoridBAKIS, VOLKAN/0000-0002-3125-9010
dc.contributor.authorBakis, V.
dc.contributor.authorBakis, H.
dc.contributor.authorBudding, E.
dc.contributor.authorDemircan, O.
dc.contributor.authorZejda, M.
dc.date.accessioned2025-01-27T20:41:42Z
dc.date.available2025-01-27T20:41:42Z
dc.date.issued2007
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionWorkshop on Solar and Stellar Physics through Eclipses -- MAR 27-29, 2006 -- Ankara Univ, ORSEM Campus, Side, Antalya, TURKEY
dc.description.abstractFirst complete BVRI light curves and radial velocity measurements of the recently discovered eclipsing binary GSC 4288 0186 are presented. Analyses of the light curves, together with spectroscopic data show that the system is a double-lined detached binary with an eccentric orbit. We determined the preliminary values of the absolute elements of this eclipsing binary and presented here.
dc.identifier.endpage+
dc.identifier.isbn978-1-583812-38-9
dc.identifier.issn1050-3390
dc.identifier.startpage213
dc.identifier.urihttps://hdl.handle.net/20.500.12428/24216
dc.identifier.volume370
dc.identifier.wosWOS:000246823600029
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofSolar and Stellar Physics Through Eclipses
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectLight Curves
dc.subjectStar Light
dc.subjectOrbit
dc.titlePhotometric and spectroscopic study of the eclipsing binary GSC 4288 0186
dc.typeConference Object

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