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Table 2
Large samples of 0.7−1.1 M⊙ stars with measured rotation periods used for comparisons with simulated rotation period distributions.
| Cluster | Age | Nstars | Reference |
| (Myr) | |||
|
|
|||
| 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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