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pro vyhledávání: '"Cora A. DeFrancesco"'
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 101 (2023)
The X-ray emission from active galactic nuclei is believed to come from a combination of inverse Compton scattering of photons from the accretion disk and reprocessing of the direct X-ray emission by reflection. We present hard (10–80 keV) and soft
Externí odkaz:
https://doaj.org/article/e392bd2529634ee3b4458ff40c05d301