On the nature of the soft γ-ray emission in the hard state of the black hole transient GRS 1716−249

ABSTRACT The black hole transient GRS 1716−249 was monitored from the radio to the γ-ray band during its 2016–2017 outburst. This paper focuses on the spectral energy distribution (SED) obtained in 2017 February–March, when GRS 1716−249 was in a bright hard spectral state. The soft γ-ray data collec...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2020-05, Vol.494 (1), p.571-583
Hauptverfasser:	Bassi, T, Malzac, J, Del Santo, M, Jourdain, E, Roques, J-P, D’Aì, A, Miller-Jones, J C A, Belmont, R, Motta, S E, Segreto, A, Testa, V, Casella, P
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics
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