Fig. 3.
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Time and angle-averaged quantities in our simulations as a function of distance from the black hole, r. The different lines denote the different configurations of the simulation. (a) Density in the units of electron number density; (b) Accretion rate Ṁ; (c) Radial velocity of the gas vr; (d) Temperature of the gas. For the density and temperature radial profiles, a line representing ∝r−1 is also plotted for reference, highlighting the approximate power law in both quantities in the inner regions of the simulations.
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