Precise Analysis of Two Kepler Detached Eclipsing Binary Stars KIC 3327980 and KIC 10156064

Basit Öğe Kaydı
dc.authoridSoydugan, Faruk/0000-0002-5141-7645
dc.contributor.authorAlicavus, Fahri
dc.contributor.authorSoydugan, Faruk
dc.date.accessioned2025-01-27T21:07:13Z
dc.date.available2025-01-27T21:07:13Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
dc.description.abstractStars are one of the most important objects to understand how the galaxies are formed; shaped and evolved. Hence, the determination of the absolute parameters of stars plays a crucial role. The absolute parameters (e.g. mass and radii) of the detached eclipsing binary stars could be determined with well accuracy. These accurate parameters could be used for understanding of the evolutional status of single stars in detailed. In this study, we carried out light curve solutions of two well-detached binaries KIC 3327980 and KIC 10156064 which were observed by Kepler space telescope. As a result, mass and radii of primary and secondary components were derived as M-1 = 1.64M(circle dot), M-2 = 1.42M(circle dot), R-1 = 2.08R(circle dot), R-2 = 1.66R(circle dot) for KIC 3327980 and M-1 = 1.67M(circle dot), M-2 = 1.05M(circle dot); R-1 = 1.92R(circle dot); R-2 = 1.06R(circle dot) for KIC 10156064. Additionally, the evolutionary status of the components of the systems were discussed and compared with the evolutional status of the other detached eclipsing binaries.
dc.description.sponsorshipTurkish Phys Soc
dc.description.sponsorshipTUBITAK (Scientific and Technological Research Council of Turkey) [111T224]; Canakkale Onsekiz Mart University Research Foundation [FDK-2016-860]
dc.description.sponsorshipThis study was supported by TUBITAK (Scientific and Technological Research Council of Turkey) under grant no, 111T224. The research was also supported by Canakkale Onsekiz Mart University Research Foundation (Project No. FDK-2016-860). This study is a part of the Ph.D. thesis of F. Alicavus. This research has made use of the SIMBAD data base, operated at CDS, Strasbourq, France.
dc.identifier.doi10.1063/1.4976435
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85015987691
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976435
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27929
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100091
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofProceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titlePrecise Analysis of Two Kepler Detached Eclipsing Binary Stars KIC 3327980 and KIC 10156064
dc.typeConference Object

Dosyalar

Koleksiyon

WoS İndeksli Yayınlar Koleksiyonu
Scopus İndeksli Yayınlar Koleksiyonu