Global Radiation-Magnetohydrodynamic Simulations of Black Hole Accretion Flow and Outflow: Unified Model of Three States
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Understanding gas accretion to the central supermassive black hole of galaxies has developed greatly and the standard disk model which appeared in the 1970s, has been extended by a slim disk model and a quasi-one-dimensional advection dominated accretion flow (ADAF) sometimes know as a radiatively inefficent accretion flow (RIAF) model....