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Fig. 8

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Comparison of the PDMFs between observations and ensemble of models en3000W6. Top panel: stars within a radius of 30 pc of the center; 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. The blue bars are derived from the observational data with N = 724 stars and lowest mass ml = 0.116   M, while the red bars are derived from the ensemble of models with  ⟨ Nf ⟩  = 736 stars and lowest mass ml = 0.08   M. The onset of incompleteness of the observations is shown as a vertical line in the top panel.

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