Fig. 11

Period versus age for early fast rotator pMS stars of the ONC. Their positions in the period-age plane are compared with models assuming evolution with constant angular momentum (Landin et al. 2006). Masses in the interval 0.2 <M/M⊙< 0.3 correspond to °, 0.3 <M/M⊙< 0.4 to ▪, and all the remaining to ×. Solid lines represent models with Jin = Jkaw, while dashed lines stand for models with Jin = 3Jkaw for M = 0.2, 0.3 and 0.4 M⊙. Figure adapted from Landin et al. (2006).
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