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Fig. 20.

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Burning Arrow results: degradation of equatorial orbits around a nonrotating BH due to the semi-opaque (LFM, Sect. 3.2d) disk’s thermal radiation. With solid black is the Bardeen et al. (1972) velocity profile, with dashed cyan and with dotted red an approximation of a SANE and a MAD model velocity profile respectively (Narayan et al. 2003, 2012; Penna et al. 2013b).

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