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Fig. B.2.
Cumulative distribution functions of stars in four different mass ranges in several key time frames (the initial conditions, t ≈ 0.5 τv, t ≈ τv and t ≈ 2 τv, given in the units of the median relaxation time, see also Fig. 5). Models with 1.2k, 2.4k, 4.7k, and 9.2k stars are plotted (from top to bottom).
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