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We carry out a time‐dependent numerical simulation where both the hydrodynamics and the radiative transfer are coupled together. We consider a two‐component accretion flow in which the Keplerian disc is immersed inside an accreting low angular momentum flow (halo) around a black hole. The injected soft photons from the Keplerian disc are reprocessed by the electrons in the halo. We show that in presence...
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