Figure 9

Figure 9: Profiles of the disk angular momentum (uϕ) for α = 0.01 (left) and α = 0.1 (right panel) for different accretion rates (as a reminder, ˙m = M˙c2∕16LEdd), showing the departures from the Keplerian profile. These plots are for a non-rotating black hole. Image reproduced by permission from [270], copyright by ESO.