GR viscous hydro simulations of Bondi-type super-Eddington flows find that black-hole mass controls whether a photon-trapped inflow-outflow structure or a convective envelope forms, with ~10% Eddington accretion onto the black hole in both cases.
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A formation scenario of black hole-envelope systems --viscous hydrodynamics simulation in general relativity--
GR viscous hydro simulations of Bondi-type super-Eddington flows find that black-hole mass controls whether a photon-trapped inflow-outflow structure or a convective envelope forms, with ~10% Eddington accretion onto the black hole in both cases.