Fig. 6
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Kinematic properties of the accretion disk according to the simulation that resembles our observations the most, taken after t = 9.62 kyr from its beginning. From left to right, the panels show the dependence with radius of the (a) mass infall rate, the (b) azimuthal velocity as a fraction of the Keplerian value, and the (c) radial velocity as a fraction of the free-fall value.
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