Photometric Study of The Eclipsing Binary ET Psc

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dc.contributor.authorOzalp, G. Z.
dc.contributor.authorOzkardes, B.
dc.date.accessioned2025-01-27T20:58:13Z
dc.date.available2025-01-27T20:58:13Z
dc.date.issued2016
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description9th International Physics Conference of the Balkan-Physical-Union (BPU) -- AUG 24-27, 2015 -- Istanbul Univ, Beyazit Campus, Istanbul, TURKEY
dc.description.abstractWe present the photometric solution of the eclipsing binary ET Psc (GSC 00608-00490). The ASAS V-band photometric data of the system was modelled using the Wilson-Devinney method. The result shows that the eclipsing pair could be classified as A-subtype of W UMa-type binary system. The absolute dimensions of the system were also estimated based on the photometric solution.
dc.description.sponsorshipBalkan Phys Union,Turkish Phys Soc
dc.identifier.doi10.1063/1.4944138
dc.identifier.isbn978-0-7354-1369-6
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-84984537194
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4944138
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26644
dc.identifier.volume1722
dc.identifier.wosWOS:000375923300019
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartof9th International Physics Conference of The Balkan Physical Union (Bpu-9)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectSky Automated Survey
dc.subjectLimb-Darkening Coefficients
dc.subjectVariable-Stars
dc.subjectCatalog
dc.titlePhotometric Study of The Eclipsing Binary ET Psc
dc.typeConference Object

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