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Fig. 4


As in Fig. 3, but showing models kept in a state of rigid rotation until approximately 1 Gyr after the TAMS. Upper panel: poMS rotational evolution for various values of α. For each α, D0 has been calibrated to obtain an optimal fit of both the subgiants and the red giants. Lower panel: the evolution of the angular momentum diffusion coefficient according to Eq. (3).

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