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Modelling the expected very high energy γ-ray emission from..:
Ducci, L
;
Romano, P
;
Vercellone, S
.
Monthly Notices of the Royal Astronomical Society. 525 (2023) 3 - p. 3923-3945 , 2023
Link:
https://doi.org/10.1093/mnras/stad2440
RT Journal T1 <Title>Modelling the expected very high energy γ-ray emission from accreting neutron stars in X-ray binaries</Title> UL https://suche.suub.uni-bremen.de/peid=cr-10.1093_mnras_stad2440&Exemplar=1&LAN=DE A1 Ducci, L A1 Romano, P A1 Vercellone, S A1 Santangelo, A PB Oxford University Press (OUP) YR 2023 SN 0035-8711 SN 1365-2966 JF Monthly Notices of the Royal Astronomical Society VO 525 IS 3 SP 3923 OP 3945 LK http://dx.doi.org/https://doi.org/10.1093/mnras/stad2440 DO https://doi.org/10.1093/mnras/stad2440 SF ELIB - SuUB Bremen
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