Fig. 10.
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Distribution of eccentricity, computed from the disk kinematics (Eqs. 5 and 6), for run R1 (a) and run R2 (b). Each curve represents a different time, with t = 0 marking the epoch of sink formation. The dashed line indicates the largest radius enclosing 90% of the disk mass over the entire simulation. The sink accretion radius is indicated by the dotted line.
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