Fig. 13
Accretion with cooling, turbulence (Ma ~ 0.35), and erot = 0.3: mid-plane Tm cross-section through z = 0 (final time). Without heating, the system experiences a massive CCA flow. Extended cold filaments and clouds condense out of the hot phase via TI, and through recurrent chaotic collisions are quickly accreted by the BH. No steady thin disk can be formed.
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