http://arxiv.org/abs/1711.08509
We study implications of the mutual interaction of a hot plasma and cold medium in black-hole binaries in their hard spectral state on the value of the truncation radii of accretion discs. We consider a number of different geometries. In contrast to previous theoretical studies, we use a modern, energy-conserving, code for reflection and reprocessing from cold media. We show that a static corona above a disc extending to the innermost stable circular orbit produces spectra not compatible with those observed. They are either too soft or require the disc ionization much higher than that observed. This conclusion confirms a number of previous findings but disproves a recent study claiming an agreement of that model with observations. We show that the cold disc has to be truncated in order to agree with the observed spectral hardness. Still, a cold disc truncated at a large radius and replaced by a hot flow produces spectra which are too hard if the only source of seed photons for Comptonization is the accretion disc. Our favourable geometry is a truncated disc coexisting with a hot plasma either overlapping with the disc or containing some cold matter within it, also including seed photons arising from cyclo-synchrotron emission of hybrid electrons, i.e., containing both thermal and non-thermal part.
J. Poutanen, A. Veledina and A. Zdziarski
Mon, 27 Nov 2017
34/78
Comments: 11 pages, 8 figures; submitted to A&A
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