Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr

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dc.contributor.authorBulut, I.
dc.date.accessioned2025-01-27T20:51:49Z
dc.date.available2025-01-27T20:51:49Z
dc.date.issued2009
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThe apsidal motion analysis of the eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr have been presented. The method described by Lacy (1992) [Lacy, C.H S.. 1992. AJ 104, 2213] has been used for the apsidal motion analysis. The apsidal motion periods have been found to be 174.2 +/- 1.4, 277.3 +/- 21.3 and 7195 +/- 174 years for V397 Cep, V493 Car and BW Aqr, respectively. (C) 2009 Elsevier B.V. All rights reserved.
dc.description.sponsorshipResearch Foundation of the Canakkale Onsekiz Mart University
dc.description.sponsorshipThe author acknowledges the partial support by Research Foundation of the Canakkale Onsekiz Mart University.
dc.identifier.doi10.1016/j.newast.2009.02.007
dc.identifier.endpage606
dc.identifier.issn1384-1076
dc.identifier.issue7
dc.identifier.scopus2-s2.0-67349101162
dc.identifier.scopusqualityQ2
dc.identifier.startpage604
dc.identifier.urihttps://doi.org/10.1016/j.newast.2009.02.007
dc.identifier.urihttps://hdl.handle.net/20.500.12428/25532
dc.identifier.volume14
dc.identifier.wosWOS:000266524200002
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier Science Bv
dc.relation.ispartofNew Astronomy
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectStars: binaries
dc.subjectStars: binaries: eclipsing
dc.subjectStars: individual: V397 Cep, V493 Car, BW Aqr
dc.titleApsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr
dc.typeArticle

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