κmonty: a Monte Carlo Compton scattering code including non-thermal electrons
ABSTRACT Low-luminosity active galactic nuclei are strong sources of X-ray emission produced by Compton scattering originating from the accretion flows surrounding their supermassive black holes. The shape and energy of the resulting spectrum depend on the shape of the underlying electron distributi...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2023-10, Vol.526 (4), p.5326-5336 |
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