Modelling the expected very high energy γ-ray emission from accreting neutron stars in X-ray binaries

dc.contributor.author	Ducci, Lorenzo
dc.contributor.author	Santangelo, Andrea
dc.date.accessioned	2024-09-16T11:52:05Z
dc.date.available	2024-09-16T11:52:05Z
dc.date.issued	2023
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10900/157492
dc.language.iso	en	de_DE
dc.publisher	Oxford : Oxford Univ Press	de_DE
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stad2440	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	Modelling the expected very high energy γ-ray emission from accreting neutron stars in X-ray binaries	de_DE
dc.type	Article	de_DE
utue.quellen.id	20240730000000_01669
utue.publikation.seiten	3923-3945	de_DE
utue.personen.roh	Ducci, L.
utue.personen.roh	Romano, P.
utue.personen.roh	Vercellone, S.
utue.personen.roh	Santangelo, A.
dcterms.isPartOf.ZSTitelID	Monthly Notices of The Royal Astronomical Society	de_DE
dcterms.isPartOf.ZS-Issue	3	de_DE
dcterms.isPartOf.ZS-Volume	525	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE