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dc.contributor.authorAyyıldız, Ömer
dc.contributor.authorAltan, Metin
dc.contributor.authorKartal, S. Utku
dc.contributor.authorHamza, Cansu
dc.contributor.authorÖzkan, M. Türker
dc.contributor.editorSchmidtobreick, L
dc.contributor.editorSchreiber, MR
dc.contributor.editorTappert, C
dc.date.accessioned2019-10-20T09:02:53Z
dc.date.available2019-10-20T09:02:53Z
dc.date.issued2011
dc.identifier.isbn978-1-58381-774-2
dc.identifier.urihttps://hdl.handle.net/11421/16555
dc.descriptionWorkshop on the Evolution of Compact Binary Stars -- MAY 06-11, 2011 -- Vina del Mar, CHILEen_US
dc.descriptionWOS: 000304125600042en_US
dc.description.abstractWe have carried out a Chandra data analysis of the prototype dwarf nova SS Cyg during quiescence and outburst. The SS Cyg data number 646 and 648 were obtained by the Chandra X-Ray Observatory on August 24, 2000 in quiescence and on September 14, 2000 in outburst were analysed. The evolution of the X-ray spectrum variation at very short periods was investigated. We discuss how situations that result from interaction are affected by the natural evolution of the system's attributes.en_US
dc.language.isoengen_US
dc.publisherAstronomical Soc Pacificen_US
dc.relation.ispartofseriesAstronomical Society of the Pacific Conference Series
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleNatural Evolution of SS Cyg Based on an X-Ray Data Analysis at Very Short Periodsen_US
dc.typeconferenceObjecten_US
dc.relation.journalEvolution of Compact Binariesen_US
dc.contributor.departmentAnadolu Üniversitesi, Fen Fakültesi, Fizik Bölümüen_US
dc.identifier.volume447en_US
dc.identifier.startpage279en_US
dc.identifier.endpage282en_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US


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