Table 1
Star-forming regions and open clusters whose rotational distributions are used is this study.
| Cluster | Age | Ref. | – | Ω25 | – | – | Ω50 | – | – | Ω90 | – | ||
| (Myr) | 1 M⊙ | 0.8 M⊙ | 0.5 M⊙ | 1 M⊙ | 0.8 M⊙ | 0.5 M⊙ | 1 M⊙ | 0.8 M⊙ | 0.5 M⊙ | ||||
|
|
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| ONC | 1.5 | 1 | 3.28 ± 0.3 | 2.86 ± 0.14 | 3.59 ± 0.26 | 4.58 ± 0.86 | 4.03 ± 0.58 | 5.27 ± 0.89 | 13.21 ± 2.14 | 20.11 ± 1.93 | 14.93 ± 3.63 | ||
| NGC 6530 | 2 | 2 | 3.87 ± 0.55 | 2.89 ± 0.19 | 3.19 ± 0.21 | 6.15 ± 0.9 | 4.08 ± 1.14 | 5.74 ± 0.54 | 22.32 ± 5.15 | 18.73 ± 2.73 | 22.72 ± 3.48 | ||
| NGC 2264 | 3 | 3 | – | 2.81 ± 0.5 | 2.81 ± 0.38 | – | 5.32 ± 0.91 | 6.16 ± 1.93 | – | 10.66 ± 2.01 | 27.57 ± 2.83 | ||
| Cep OB3b | 4 | 4 | 3.25 ± 0.39 | 3.91 ± 0.81 | 3.38 ± 0.2 | 6.99 ± 1.07 | 6.45 ± 1 | 5.58 ± 0.43 | 14.98 ± 1.55 | 17.13 ± 2.14 | 23.66 ± 5.42 | ||
| NGC 2362 | 5 | 5 | 3.13 ± 0.29 | 2.75 ± 0.29 | 3.9 ± 0.26 | 4.2 ± 0.58 | 3.82 ± 0.29 | 6.31 ± 0.67 | 12.36 ± 4.76 | 14.01 ± 4.4 | 23.09 ± 5.94 | ||
| h Per | 13 | 6 | 4.75 ± 0.19 | 3.93 ± 0.17 | 4.5 ± 0.53 | 8.31 ± 0.85 | 6.33 ± 0.74 | 11.93 ± 5.03 | 73.37 ± 6.32 | 46.99 ± 6.2 | 58.4 ± 4.37 | ||
| NGC 2547 | 35 | 7 | – | 4.55 ± 0.38 | 4.77 ± 0.87 | – | 5.28 ± 1.01 | 10.82 ± 1.86 | – | 47.31 ± 22.35 | 45.24 ± 17.7 | ||
| IC 2391 | 50 | 8 | – | 4.38 ± 0.76 | – | – | 9.76 ± 4.29 | – | – | 98.13 ± 31.77 | – | ||
| α Per | 80 | 8 | – | 5.88 ± 0.75 | – | – | 14.81 ± 8.32 | – | – | 98.41 ± 14.26 | – | ||
| Pleiades | 125 | 9 | 4.92 ± 0.13 | 3.59 ± 0.08 | 7.98 ± 1.2 | 6.29 ± 0.31 | 4.27 ± 0.24 | 18.24 ± 1.91 | 37.99 ± 10.08 | 61.49 ± 5.5 | 76.74 ± 4.91 | ||
| M 50 | 130 | 10 | 3.38 ± 0.3 | 3.21 ± 0.1 | 6.79 ± 0.53 | 5.17 ± 0.36 | 4.23 ± 0.22 | 17.19 ± 1.74 | 15.41 ± 5.16 | 43.12 ± 3.55 | 72.22 ± 3.32 | ||
| M 35 | 150 | 11 | 4.39 ± 0.07 | 3.38 ± 0.1 | – | 5.05 ± 0.22 | 4.59 ± 0.71 | – | 24.3 ± 5.27 | 59.3 ± 5.55 | – | ||
| NGC 2516 | 150 | 12 | – | – | 5.11 ± 0.66 | – | – | 11.52 ± 1.56 | – | – | 70.12 ± 4.39 | ||
| M 34 | 220 | 13 | 3.68 ± 0.14 | 2.67 ± 0.1 | – | 4.64 ± 0.83 | 3.07 ± 0.09 | – | 27.02 ± 6.78 | 21.31 ± 5.14 | – | ||
| M 37 | 550 | 14 | 2.95 ± 0.05 | 2.38 ± 0.04 | 1.97 ± 0.44 | 3.26 ± 0.06 | 2.63 ± 0.06 | 11.23 ± 3.37 | 3.75 ± 0.13 | 3.7 ± 0.27 | 40.69 ± 2.14 | ||
| Praesepe | 580 | 15 | 2.73 ± 0.05 | 2.11 ± 0.05 | 1.39 ± 0.07 | 2.85 ± 0.02 | 2.52 ± 0.11 | 3.28 ± 1.57 | 2.92 ± 0.75 | 5.94 ± 1.39 | 22.03 ± 4.63 | ||
| Hyades | 625 | 16 | 2.44 ± 0.03 | 2.05 ± 0.04 | 1.41 ± 0.07 | 2.62 ± 0.06 | 2.18 ± 0.03 | 1.91 ± 0.09 | 2.91 ± 0.1 | 2.46 ± 0.15 | 2.3 ± 0.78 | ||
| NGC 6811 | 1000 | 17 | 2.27 ± 0.04 | – | – | 2.36 ± 0.01 | – | – | 2.45 ± 0.05 | – | – | ||
Reference. (1) Rodríguez-Ledesma et al. (2009); (2) Henderson & Stassun (2012); (3) Cieza & Baliber (2007); (4) Littlefair et al. (2010); (5) Irwin et al. (2008a); (6) Moraux et al. (2013); (7) Irwin et al. (2008b); (8) Irwin et Bouvier; (9) Hartman et al. (2010); (10) Irwin et al. (2009); (11) Meibom et al. (2009); (12) Irwin et al. (2007); (13) Meibom et al. (2011b); (14) Hartman et al. (2009); (15) Agüeros et al. (2011)+Delorme et al. (2011); (16) Delorme et al. (2011); (17) Meibom et al. (2011a).
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