A light and period study of SV Camelopardalis

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dc.contributor.authorAlbayrak, B
dc.contributor.authorDemircan, O
dc.contributor.authorDjurasevic, G
dc.contributor.authorErkapic, S
dc.contributor.authorAk, H
dc.date.accessioned2025-01-27T20:59:59Z
dc.date.available2025-01-27T20:59:59Z
dc.date.issued2001
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractNew BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analysed to derive the physical parameters of the system and the parameters of the third body orbit. The light curves obtained at the TUBITAK National Observatory during two nights in 2000 show considerable asymmetry and night-to-night variations. The analysis of the light curves is made using Djurasevic's inverse problem method. The Roche model with spotted areas on the hotter primary component yields a good fit to observations. The extensive series of published photoelectric minima times indicate that the eclipsing pair orbits around the common mass center of the triple system with a period of 41.32 yr.
dc.identifier.doi10.1051/0004-6361:20010914
dc.identifier.endpage164
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.issue1
dc.identifier.scopus2-s2.0-0035443648
dc.identifier.scopusqualityQ1
dc.identifier.startpage158
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20010914
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26900
dc.identifier.volume376
dc.identifier.wosWOS:000170646600021
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherEdp Sciences S A
dc.relation.ispartofAstronomy & Astrophysics
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectstars : binaries : eclipsing
dc.subjectstars : individual : SV Cam
dc.titleA light and period study of SV Camelopardalis
dc.typeArticle

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