Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte Carlo approach

dc.contributor.author	Suleimanov, Valery F.
dc.date.accessioned	2021-11-05T14:07:38Z
dc.date.available	2021-11-05T14:07:38Z
dc.date.issued	2021
dc.identifier.issn	1365-2966
dc.identifier.uri	http://hdl.handle.net/10900/120507
dc.language.iso	en	de_DE
dc.publisher	Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stab811	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte Carlo approach	de_DE
dc.type	Article	de_DE
utue.quellen.id	20210824232002_01041
utue.publikation.seiten	5193-5203	de_DE
utue.personen.roh	Mushtukov, Alexander A.
utue.personen.roh	Suleimanov, Valery F.
utue.personen.roh	Tsygankov, Sergey S.
utue.personen.roh	Zwart, Simon Portegies
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	4	de_DE
dcterms.isPartOf.ZS-Volume	503	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE