Fig. 11
Left: slope of the log P− mass relationship as a function of age recovered from the simulations (green dots) and superimposed to data points from Henderson & Stassun (2012) for seven nearby clusters. The error bars of the green dots are equal to the standard errors of the estimate of the least-squares fits. Right: same plot for a modified model without disk locking for the 0.3 M⊙ stars.
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