Magnetospheric flows in X-ray pulsars - I. Instability at super-Eddington regime of accretion

dc.contributor.author	Suleimanov, Valery F.
dc.date.accessioned	2025-03-12T15:09:04Z
dc.date.available	2025-03-12T15:09:04Z
dc.date.issued	2024
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10900/162900
dc.language.iso	en	en
dc.publisher	Oxford : Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stae781
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Magnetospheric flows in X-ray pulsars - I. Instability at super-Eddington regime of accretion	de_DE
dc.type	Article	de_DE
utue.quellen.id	20241001000000_02003
utue.publikation.seiten	730-742	de_DE
utue.personen.roh	Mushtukov, A. A.
utue.personen.roh	Ingram, A.
utue.personen.roh	Suleimanov, V. F.
utue.personen.roh	Dilullo, N.
utue.personen.roh	Middleton, M.
utue.personen.roh	Tsygankov, S. S.
utue.personen.roh	van der Klis, M.
utue.personen.roh	Portegies Zwart, S.
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	1	de_DE
dcterms.isPartOf.ZS-Volume	530	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät