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Escape probability methods versus “exact" transfer for modelling the X-ray spectrum of Active Galactic Nuclei and X-ray binaries
In the era of XMM-Newton and Chandra missions, it is crucial to use codes able to compute correctly the line spectrum of X-ray irradiated thick media (Thomson thickness of the order of unity) to build models for the structure and the emission of the central regions of AGN or X-ray …