Light curve, analyses of new eclipsing binary systems with eccentric orbits

dc.contributor.authorBulut, I.
dc.contributor.authorDemircan, O.
dc.date.accessioned2025-01-27T21:13:09Z
dc.date.available2025-01-27T21:13:09Z
dc.date.issued2008
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractA photometric study of seven new eclipsing binary systems with eccentric orbits, namely, V466 Car, V493 Car, V529 Car, MN TrA, V398 Lac, V402 Lac and V821 Cas, is presented. The photometric data analyzed were taken from the Hipparcos database. The secondary minima in all systems were shifted by different amounts from the phase 0.5 giving clear evidence of their eccentric orbits. The EBOP computer program based upon models by Nelson et al. [Popper, D.M., Etzel, P.E., 1981. AJ 86, 102] was used in the analysis of the photometric data to deduce the orbital geometry in space and the relative sizes and luminosities of the component stars. (C) 2007 Elsevier B.V. All rights reserved.
dc.identifier.doi10.1016/j.newast.2007.10.003
dc.identifier.endpage254
dc.identifier.issn1384-1076
dc.identifier.issue4
dc.identifier.scopus2-s2.0-36749038806
dc.identifier.scopusqualityQ2
dc.identifier.startpage252
dc.identifier.urihttps://doi.org/10.1016/j.newast.2007.10.003
dc.identifier.urihttps://hdl.handle.net/20.500.12428/28312
dc.identifier.volume13
dc.identifier.wosWOS:000252833300007
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 : close
dc.subjectstars : binaries : eclipsing
dc.subjectstars : individual : V466 car
dc.subjectV493 Car
dc.subjectV529 Car
dc.subjectMN TrA
dc.subjectV398 Lac
dc.subjectV402 Lac
dc.subjectV821 Cas
dc.titleLight curve, analyses of new eclipsing binary systems with eccentric orbits
dc.typeArticle

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