Light-Time Effect in Two Eclipsing Binaries: NO Vul and EW Lyr

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dc.contributor.authorBulut, A.
dc.contributor.authorBulut, I.
dc.contributor.authorCicek, C.
dc.contributor.authorErdem, A.
dc.date.accessioned2025-01-27T20:50:16Z
dc.date.available2025-01-27T20:50:16Z
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.abstractIn this study, orbital period variations of two eclipsing binary systems (NO Vul and EW Lyr) were discussed. Possible light time effects due to third bodies in these systems were re-examined. The mass function and orbital period of hypothetical third bodies were calculated to be 0.000627 +/- 1.000003 M-circle dot, 26.17 +/- 0.05 years and 0.12682 +/- 0.00003 M-circle dot, 77.23 +/- 0.72 years for NO Vul and EW Lyr, respectively.
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.4976438
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85015992504
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976438
dc.identifier.urihttps://hdl.handle.net/20.500.12428/25456
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100094
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.subjectbinaries
dc.subjecteclipsing
dc.subjectlight-time effect
dc.subjectstars: individual: NO Vul and EW Lyr
dc.titleLight-Time Effect in Two Eclipsing Binaries: NO Vul and EW Lyr
dc.typeConference Object

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