Fig. 3.
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SKIRT radiative transfer modelling of the Fe Kα line in the radiation-driven fountain model of Wada et al. (2016), representing the cold gas around the Circinus AGN. Right: Normalised Fe Kα line profiles for different inclinations. The velocity broadening of the Fe Kα line is significant and can only be modelled when the intrinsic line profiles are taken into account. Left: Broadband spectrum and red-green-blue image for i = 90°.
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