Third body problem in the eclipsing binary star TV Cassiopeia

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dc.contributor.authorErdem, A
dc.date.accessioned2025-01-27T20:12:10Z
dc.date.available2025-01-27T20:12:10Z
dc.date.issued2002
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionNATO Advances Study Institute Conference on RestlessUniverse -- JUL 23-AUG 05, 2000 -- BLAIR ATHOLL, SCOTLAND
dc.description.abstractThe aim of this work is to search for some evidences for the presence of unseen companion(s) in the eclipsing binary star TV Cassiopeia using its O-C diagram. Assuming that the light-time effect is responsible for the periodic components on the O-C diagram, the set of orbital parameters were derived using Irwin's (1959) method. The resulting orbital parameters and mass of the hypothetical third body are physically acceptable. Lacking other proofs of the third body presence, however, the hypothesis can be treated as a probable case only.
dc.description.sponsorshipNATO
dc.identifier.doi10.1023/A:1014560600056
dc.identifier.endpage141
dc.identifier.issn0923-2958
dc.identifier.issue2
dc.identifier.scopus2-s2.0-0141569396
dc.identifier.scopusqualityQ2
dc.identifier.startpage133
dc.identifier.urihttps://doi.org/10.1023/A:1014560600056
dc.identifier.urihttps://hdl.handle.net/20.500.12428/20864
dc.identifier.volume82
dc.identifier.wosWOS:000174253700003
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofCelestial Mechanics & Dynamical Astronomy
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjecteclipsing binaries
dc.subjectTV Cas
dc.subjectorbital period variation
dc.subjectthird body problem
dc.titleThird body problem in the eclipsing binary star TV Cassiopeia
dc.typeConference Object

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