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

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

Author: Ducci, L.; Romano, P.; Vercellone, S.; Santangelo, A.
Tübinger Autor(en):
Ducci, Lorenzo
Santangelo, Andrea
Published in: Monthly Notices of The Royal Astronomical Society (2023), Bd. 525, H. 3, S. 3923-3945
Verlagsangabe: Oxford : Oxford Univ Press
Language: English
Full text: http://dx.doi.org/10.1093/mnras/stad2440
ISSN: 0035-8711
DDC Classifikation: 520 - Astronomy and allied sciences
530 - Physics
Dokumentart: Article
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