Accretion of a clumped wind from a red supergiant donor on to a magnetar is suggested by the analysis of the XMM-Newton and NuSTAR observations of the X-ray binary 3A 1954+319

dc.contributor.author	Ducci, Lorenzo
dc.date.accessioned	2023-01-13T13:32:02Z
dc.date.available	2023-01-13T13:32:02Z
dc.date.issued	2022
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10900/135349
dc.language.iso	en	de_DE
dc.publisher	Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stab3688	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Accretion of a clumped wind from a red supergiant donor on to a magnetar is suggested by the analysis of the XMM-Newton and NuSTAR observations of the X-ray binary 3A 1954+319	de_DE
dc.type	Article	de_DE
utue.quellen.id	20220728000000_01730
utue.publikation.seiten	4645-4653	de_DE
utue.personen.roh	Bozzo, E.
utue.personen.roh	Ferrigno, C.
utue.personen.roh	Oskinova, L.
utue.personen.roh	Ducci, L.
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	3	de_DE
dcterms.isPartOf.ZS-Volume	510	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE

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