Photometric Analysis of Kepler Contact Binaries With Large Fill-Out Factors: KIC 3221207 and KIC 6677225

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dc.authoridSoydugan, Faruk/0000-0002-5141-7645
dc.contributor.authorAlicavus, Fahri
dc.contributor.authorSoydugan, Faruk
dc.date.accessioned2025-01-27T20:27:05Z
dc.date.available2025-01-27T20:27:05Z
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.abstractContact binary stars have an important role to understand how the binary stars evolve to a single star and explain to the physical processes of star merges. Hence, understanding of different type of contact binaries is valuable to explore sonic physical processes such as angular momentum loses, mass and heat transfers between components. In this study, we present the photometric analysis of two Kepler binary stars KIC 3221207 and KIC 6677225. As a result, it was found that both eclipsing binaries have large amount of common envelopes. The till-out factors of stars were determined to be 79 and 89 percent for KIC 3221207 and KIC 6677225, respectively. Furthermore, both systems show parabolic orbital period variations, while the third light contribution was found for KIC 3221207. In the result, we compare the target systems with similar, well-known contact binaries.
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.4976436
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85015989806
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976436
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22575
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100092
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.subjectEclipsing Binaries
dc.subjectVariable-Stars
dc.subjectCatalog
dc.titlePhotometric Analysis of Kepler Contact Binaries With Large Fill-Out Factors: KIC 3221207 and KIC 6677225
dc.typeConference Object

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