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Fig. 7.
Evolution of the 0.2, 0.5 (thick line), and 0.75 Lagrangian radius of the star cluster models. Shown are the lower (Mcl(0) = 1400 M⊙) and higher mass (Mcl(0) = 4400 M⊙) clusters, (left and right panels, respectively). The age of the Pleiades is indicated by the vertical yellow line.
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