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Table 1.
Open clusters with age determinations and measured rotation period distributions used for deriving the best fit parameters of the parametric model of rotation evolution.
| Open cluster | Age (Myr) | Reference (age determination) | Nstars (0.9–1.1 M⊙) | Reference (rotation measurements) |
|---|---|---|---|---|
| Pleiades | 112 ± 5 | Dahm 2015 | 75 | Hartman et al. 2010 |
| M50 | ~130 | Kalirai et al. 2003 | 61 | Irwin et al. 2009 |
| M35 | ~133 | McNamara et al. 2011 | 110 | Meibom et al. 2009 |
| M37 | 550 ± 30 | Hartman et al. 2008 | 88 | Hartman et al. 2009 |
| NGC 6811 | 1050 ± 140 | Sandquist et al. (2016) | 34 | Meibom et al. 2011 |
| NGC 6819 | 2380 ± 270 | Brewer et al. (2016) | 16 | Meibom et al. 2015 |
| M67 |  |
VandenBerg et al. 2004 | 8 | Barnes et al. 2016 |
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