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Fig. 1.

Simulated evolution of a normal rotation period distribution of solar mass stars compared with measured rotation period histograms of 0.9–1.1 M⊙ stars in the Pleiades (112 Myr), M50 and M35 (130 Myr), M37 (550 Myr), NGC 6811 (1050 Myr), NGC 6819 (2380 Myr), and M67 (4000 Myr).
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