Proc. IAU volume 13, issue S336, P135-136 2017 DOI: 10.1017/s1743921317010043 View full text
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E. Fedorova, B. I. Hnatyk, V. I. Zhdanov, A. Vasylenko

Abstract: AbstractMapping the maser emission of subnuclear regions of active galactic nuclei (AGN) enable us to determine some interesting details of the geometry of the accretion disks (AD) under the condition that they have “maser skin”. Additional information about disk warp in the innermost zone near the central black hole (BH) can be disclosed by means of modeling the shape of the relativistically broadened iron emission lines in the energy range 6-7 keV. Here we analyze the influence of the AD geometry (warp) on t…

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