Table 1
Open clusters whose rotational distributions are used is this study.
| Cluster | Age | N star | Mass bin | Ref. | Ω25 | Ω50 | Ω90 |
| (Myr) | (M⊙) | – | (Ω⊙) | – | |||
|
|
|||||||
| ONC | 1 | 154 | 0.25−1.2 | 1 | 2.88 ± 0.07 | 3.73 ± 0.16 | 17.64 ± 1.61 |
| NGC 6530 | 1.65 | 129 | 0.5−1.1 | 2 | 3.43 ± 0.26 | 6.14 ± 0.47 | 22.25 ± 2.64 |
| NGC 2264 | 2 | 41 | 0.6−1.2 | 3 | 4.03 ± 0.49 | 6.74 ± 0.49 | 11.37 ± 1.28 |
| NGC 2362 | 5 | 64 | 0.8−1.1 | 4 | 2.78 ± 0.26 | 3.79 ± 0.36 | 12.34 ± 2.61 |
| h PER | 13 | 159 | 0.8−1.1 | 5 | 4.27 ± 0.27 | 6.54 ± 0.7 | 60.66 ± 7.33 |
| NGC 2547 | 40 | 47 | 0.6−1.1 | 6 | 4.51 ± 0.26 | 5.76 ± 1.05 | 51.01 ± 12.57 |
| Pleiades | 120 | 74 | 0.9−1.1 | 7 | 4.96 ± 0.13 | 6.21 ± 0.31 | 38 ± 9.92 |
| M 50 | 130 | 62 | 0.9−1.1 | 8 | 3.81 ± 0.31 | 5.21 ± 0.33 | 36.34 ± 19.02 |
| M 35 | 150 | 70 | 0.9−1.1 | 9 | 4.39 ± 0.09 | 5.25 ± 0.2 | 22.28 ± 5.03 |
| M 37 | 550 | 75 | 0.9−1.1 | 10 | 2.95 ± 0.05 | 3.26 ± 0.06 | 3.75 ± 0.16 |
| Praesepe | 578 | 12 | 0.9−1.1 | 11 | 2.54 ± 0.05 | 2.68 ± 0.04 | 2.73 ± 0.03 |
| Hyades | 625 | 7 | 0.9−1.1 | 11 | 2.48 ± 0.07 | 2.68 ± 0.06 | 2.91 ± 0.1 |
| NGC 6811 | 1000 | 31 | 0.9−1.1 | 12 | 2.25 ± 0.02 | 2.33 ± 0.02 | 2.39 ± 0.02 |
Reference. (1) Herbst et al. (2002); (2) Henderson & Stassun (2012); (3) Affer et al. (2013); (4) Irwin et al. (2008a); (5) Moraux et al. (2013); (6) Irwin et al. (2008b); (7) Hartman et al. (2010); (8) Irwin et al. (2009); (9) Meibom et al. (2009); (10) Hartman et al. (2009); (11) Delorme et al. (2011); (12) Meibom et al. (2011).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.