The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

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dc.contributor.author Suleimanov, Valery F.
dc.date.accessioned 2015-05-28T13:30:56Z
dc.date.available 2015-05-28T13:30:56Z
dc.date.issued 2014
dc.identifier.issn 0035-8711
dc.identifier.uri http://hdl.handle.net/10900/63423
dc.language.iso en de_DE
dc.publisher Oxford Univ Press de_DE
dc.relation.uri http://dx.doi.org/10.1093/mnras/stu2073 de_DE
dc.rights info:eu-repo/semantics/closedAccess
dc.subject.ddc 520 de_DE
dc.subject.ddc 530 de_DE
dc.title The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts de_DE
dc.type Artikel de_DE
utue.quellen.id 20150423052756_00017 de_DE
utue.publikation.seiten 4218-4234 de_DE
utue.personen.roh Kajava, Jari J. E.
utue.personen.roh Nattila, Joonas
utue.personen.roh Latvala, Outi-Marja
utue.personen.roh Pursiainen, Miika
utue.personen.roh Poutanen, Juri
utue.personen.roh Suleimanov, Valery F.
utue.personen.roh Revnivtsev, Mikhail G.
utue.personen.roh Kuulkers, Erik
utue.personen.roh Galloway, Duncan K.
dcterms.isPartOf.ZSTitelID Monthly Notices of The Royal Astronomical Society de_DE
dcterms.isPartOf.ZS-Issue 4 de_DE
dcterms.isPartOf.ZS-Volume 445 de_DE
utue.fakultaet 07 Mathematisch-Naturwissenschaftliche Fakultät de_DE


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