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

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

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 collected wit...

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Bibliographic Details
Main Authors: Bassi, T., Malzac, J., Del Santo, M., Jourdain, E., Roques, J.P., D'Aì, A., Miller-Jones, James, Belmont, R., Motta, S.E., Segreto, A., Testa, V., Casella, P.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2020
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
accretion, accretion discs
black hole physics
ISM: jets and outflows
gammarays: general
X-rays: binaries
SPECTRAL ENERGY-DISTRIBUTION
X-RAY
COMPACT JET
INTERNAL SHOCKS
CYGNUS X-1
ACCRETION
RADIO
VARIABILITY
SYNCHROTRON
RADIATION
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91531

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91531

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