The Light Curve Analysis of The Highly Eccentric Eclipsing Binary KIC 10296163

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dc.contributor.authorCicek, C.
dc.contributor.authorBulut, A.
dc.contributor.authorBulut, I
dc.date.accessioned2025-01-27T21:07:15Z
dc.date.available2025-01-27T21:07:15Z
dc.date.issued2019
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description35th International Physics Congress of the Turkish-Physical-Society (TPS) -- SEP 04-08, 2019 -- Bodrum, TURKEY
dc.description.abstractIn this study, the analysis of the Kepler light curve of the eclipsing binary KIC 10296163 (Gaia DR2 2085670964017513856, R.A.(2000) = 19(h)564(m)40(s).07, DEC2000 = +47(0) 21'21 ''.97, m(R) = 13.43 mag) is presented. The light curve of the system shows a secondary minimum from a shifted phase 0.5 which indicates the ellipticity of the orbit. By using the PHOEBE program we analysed the light curve to achieve the orbital parameters of the system. The results of our analysis indicates a detached system where the orbit is highly eccentric (e = 0.357 +/- 0.003). Therefore, KIC 11858541 is a suitable candidate for apsidal motion studies.
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.5135471
dc.identifier.isbn978-0-7354-1925-4
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85076469295
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.5135471
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27950
dc.identifier.volume2178
dc.identifier.wosWOS:000618879700074
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofTurkish Physical Society 35th International Physics Congress (Tps35)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titleThe Light Curve Analysis of The Highly Eccentric Eclipsing Binary KIC 10296163
dc.typeConference Object

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