Potential origin of the state-dependent high-energy tail in the black hole microquasar Cygnus X-1 as seen with INTEGRAL

dc.contributor.author	Grinberg, Victoria
dc.date.accessioned	2021-10-14T08:06:13Z
dc.date.available	2021-10-14T08:06:13Z
dc.date.issued	2021
dc.identifier.issn	1432-0746
dc.identifier.uri	http://hdl.handle.net/10900/119610
dc.language.iso	en	de_DE
dc.publisher	Edp Sciences S A	de_DE
dc.relation.uri	http://dx.doi.org/10.1051/0004-6361/202038604	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Potential origin of the state-dependent high-energy tail in the black hole microquasar Cygnus X-1 as seen with INTEGRAL	de_DE
dc.type	Article	de_DE
utue.quellen.id	20210824232002_00707
utue.personen.roh	Cangemi, F.
utue.personen.roh	Beuchert, T.
utue.personen.roh	Siegert, T.
utue.personen.roh	Rodriguez, J.
utue.personen.roh	Grinberg, V
utue.personen.roh	Belmont, R.
utue.personen.roh	Gouiffes, C.
utue.personen.roh	Kreykenbohm, I
utue.personen.roh	Laurent, P.
utue.personen.roh	Pottschmidt, K.
utue.personen.roh	Wilms, J.
dcterms.isPartOf.ZSTitelID	Astronomy & Astrophysics	de_DE
dcterms.isPartOf.ZS-Issue	Article A93	de_DE
dcterms.isPartOf.ZS-Volume	650	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE