The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei

The hard X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries is thought to be produced by a hot cloud of electrons referred to as the corona. This emission, commonly described by a power law with a high-energy cutoff, is suggestive of Comptonization by thermal electrons. Whi...

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Veröffentlicht in:	arXiv.org 2023-11
Hauptverfasser:	Kammoun, E, Lohfink, A M, Masterson, M, Wilkins, D R, Zhao, X, Baloković, M, Boorman, P G, Connors, R M T, Coppi, P, Fabian, A C, García, J A, Madsen, K K, N Rodriguez Cavero, Sridhar, N, Stern, D, Tomsick, J, Wevers, T, Walton, D J, Bianchi, S, Buchner, J, Civano, F, Lanzuisi, G, Mallick, L, Matt, G, Merloni, A, Nardini, E, Piotrowska, J M, Ricci, C, K -W Wong, Zoghbi, A, the HEX-P Collaboration
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Black holes Electron distribution Electrons Emission analysis Evolution High energy astronomy Luminosity Quasars Sensitivity Spatial resolution Universe X ray binaries X ray imagery X ray stars X-ray astronomy
Online-Zugang:	Volltext
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