Black hole accretion at 0.6 times the Eddington rate can form a stable puffy disk, with a thin dense core, a thick Keplerian photosphere, and most inflow above the core.
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Puffy accretion disks: sub-Eddington, optically thick, and stable
Black hole accretion at 0.6 times the Eddington rate can form a stable puffy disk, with a thin dense core, a thick Keplerian photosphere, and most inflow above the core.