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dc.contributor.authorKalomeni, Belinda
dc.date.accessioned2017-03-06T08:05:51Z
dc.date.available2017-03-06T08:05:51Z
dc.date.issued2011
dc.identifier.citationKalomeni, B. (2011, August 2-6). Evolution of binaries towards HMXBs and LMXBs. Paper presented at the Conference on Astrophysics of Neutron Stars in Honor of M Ali Alpar (ASTRONS). doi:10.1063/1.3629516en_US
dc.identifier.isbn9780735409392
dc.identifier.issn0094-243X
dc.identifier.urihttp://doi.org/10.1063/1.3629516
dc.identifier.urihttp://hdl.handle.net/11147/4975
dc.descriptionAstrophysics of Neutron Stars 2010 - A Conference in Honor of M. Ali Alpar; Cesme, Izmir; Turkey; 2 August 2010 through 6 August 2010en_US
dc.description.abstractIn this study we investigate the evolution of binary systems towards low mass x-ray binaries and high mass x-ray binaries using Eggleton's binary star evolution code. © 2011 American Institute of Physics.en_US
dc.language.isoengen_US
dc.publisherAmerican Institute of Physics Publisingen_US
dc.relation.isversionof10.1063/1.3629516en_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectBinary systemsen_US
dc.subjectHMXBsen_US
dc.subjectLMXBsen_US
dc.subjectStellar evolutionen_US
dc.titleEvolution of binaries towards HMXBs and LMXBsen_US
dc.typeconferenceObjecten_US
dc.contributor.authorIDTR17457en_US
dc.contributor.institutionauthorKalomeni, Belinda
dc.relation.journalAIP Conference Proceedingsen_US
dc.contributor.departmentİYTE, Fen Fakültesi, Fizik Bölümüen_US
dc.identifier.volume1379en_US
dc.identifier.startpage204en_US
dc.identifier.endpage205en_US
dc.identifier.wosWOS:000302936600041
dc.identifier.scopusSCOPUS:2-s2.0-80053374566
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US


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