X-ray and Gamma-ray Emission from a High-Temperature Plasma and the Spectra of Accreting Black Holes

arXiv:2607.07582 · astro-ph.HE · Submitted 2026-07-08 · Read on arXiv

S. A. Grebenev

Space Research Institute, Moscow

astro-ph.HE

Submitted: 2026-07-08

Comments: 37 pages, 22 figures, 3 tables

Journal ref: Astronomy Letters, 51 (2025), 655-691

DOI: 10.1134/S106377372670009X

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Accuracy — 2× in this paper · explained in 1 episode
• alpha — 2× in this paper · explained in 1 episode
• Absorption Cross Section — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Trace — 1× in this paper · explained in 2 episodes

Sources

• X-ray nova MAXI J1828-249. Evolution of the broadband spectrum during its 2013-2014 outburst
• Discovery of Strong Energy-Dependent X-ray Polarization in the Intermediate State of GS 1354-64

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