Fig. 26

Core radius (heavy black line) and Lagrangian radii containing 90%, 80%, 70%, 60%, 50%, 40%, 30%, 20%, 10%, 5%, and 3% (dashed lines from top to bottom) of the total mass. The half mass radius is indicated by a heavier dashed line. The initial condition was a King model with W0 = 6 containing 6144 stars. A Scalo mass function with mass limits mlower = 0.1 M⊙ and mupper = 100 M⊙ was chosen as the initial mass function. Core collapse is reached at tcc ≃ 20.6 N-body time units or tcc ≃ 0.21trlx, which is the time of formation of the first hard binary.
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