Large samples of 0.7−1.1 M⊙ stars with measured rotation periods used for comparisons with simulated rotation period distributions.
|NGC 2362||5||91||Irwin et al. (2008)|
|h Per||13||207||Moraux et al. (2013)|
|Pleiades||125||170||Hartman et al. (2010)|
|M 50||130||316||Irwin et al. (2009)|
|M 35||133||223||Meibom et al. (2009)|
|M 37||550||284||Hartman et al. (2009)|
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