Fig. 16
Comparison of the PDMFs between ensembles enb2250PL, en2250PL, and enb2125PL. Top panel: stars within a radius of 30 pc of the center (Jacobi radius); middle panel: stars within a radius of 9 pc of the center (Jacobi radius); bottom panel: stars within a radius of 3 pc of the center (core). Shown is the mean value of log (N) from the ensemble averaging over 15 runs. The errors are 1σm standard errors.
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