The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

dc.contributor.author	Werner, Klaus
dc.contributor.author	Suleimanov, Valery F.
dc.date.accessioned	2018-02-07T14:21:03Z
dc.date.available	2018-02-07T14:21:03Z
dc.date.issued	2017
dc.identifier.issn	1365-2966
dc.identifier.uri	http://hdl.handle.net/10900/80178
dc.language.iso	en	de_DE
dc.publisher	Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stw3132	de_DE
dc.rights	info:eu-repo/semantics/closedAccess
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii	de_DE
dc.type	Article	de_DE
utue.quellen.id	20170815222223_01321
utue.publikation.seiten	906-913	de_DE
utue.personen.roh	Suleimanov, Valery F.
utue.personen.roh	Poutanen, Juri
utue.personen.roh	Nattila, Joonas
utue.personen.roh	Kajava, Jari J. E.
utue.personen.roh	Revnivtsev, Mikhail G.
utue.personen.roh	Werner, Klaus
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	1	de_DE
dcterms.isPartOf.ZS-Volume	466	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE