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Fig. 18


Initial distribution of periods at 5 Myr (top panels) for 0.6–0.9 M stars is projected to 13 and 130 Myr (top to bottom panels) using three models: strong core-envelope coupling (τc = 1 Myr, left panels), weak core-envelope coupling (τc = 50 Myr, middle panels), and a velocity-dependent coupling timescale (τc = 500 (ω/ω)-1 Myr, right panels). The observed distributions are shown as black shaded histograms, the projected ones as red bar histograms.

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