Fig. 2.
Synthetic slow-rotator sequences predicted by our two-zone model at 120 Myr, 700 Myr, and 1 Gyr (red solid lines with stars) compared with the observations (colored circles). The black circles with error bars represent qualitative fits of the slow-rotator sequences; the error bars shown are 1.5 days for the Pleiades sequence and 1 day for Praesepe and NGC 6811.
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