Fig. 6.
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Time evolution of the Lagrangian radii of two stellar mass groups: low-mass (‘L’, m ≤ 0.2 M⊙, dotted lines) and high-mass (‘H’, m ≥ 0.9 M⊙, solid lines). The curves represent 1, 50, 75, and 90% of the total mass of the corresponding mass group (from bottom to top; the half-mass radius is also highlighted in red). The cluster tidal radius is the top dashed line.
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