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

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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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