Table 3
Rotation periods, inclination angle, and Rossby numbers for the 22 stars computed with different approaches.
Ref. no | KIC | Prot (days) | i (°) | R ol | R og | Ro (N84) | dCZ (R) | ||
|
|||||||||
1 | 1430163 | 3.88 ± 0.58 | 31.75 ± 7.57 | 1.54 | |||||
2 | 1435467 | 6.53 ± 0.64 | 47.08 ± 10.92 | 3.026 | 2.248 | 5.14 | 0.12 | ||
3 | 3733735 | 2.54 ± 0.16 | 31.41 ± 3.52 | 11.964 | 8.762 | 2.08 | 0.05 | ||
4 | 4638884 | 6.17 ± 0.60 | 27.23 ± 5.27 | 2.65 | |||||
5 | 5371516 | 5.13 ± 0.48 | 47.63 ± 9.21 | 1.68 | |||||
6 | 5773345 | 11.60 ± 0.90 | 47.47 ± 11.97 | 4.24 | |||||
7 | 6508366 | 3.78 ± 0.34 | 36.92 ± 5.50 | 2.20 | |||||
8 | 7103006 | 4.61 ± 0.38 | 35.70 ± 5.46 | 1.21 | |||||
9 | 7206837 | 4.04 ± 0.25 | 29.76 ± 4.06 | 1.269 | 1.036 | 2.38 | 0.13 | ||
10 | 7668623 | 5.12 ± 0.38 | 25.13 ± 3.73 | 0.99 | |||||
11 | 7771282 | 11.91 ± 0.96 | ... | 40.93 | |||||
12 | 7940546 | 11.12 ± 0.85 | 90 ± 20 | 4.21 | |||||
13 | 8026226 | 11.14 ± 2.16 | 47.57 ± 19.80 | 4.17 | |||||
14 | 9226926 | 2.17 ± 0.14 | 50.31 ± 6.20 | 2.59 | |||||
15 | 9289275 | 11.31 ± 1.02 | ... | 2.99 | |||||
16 | 9812850 | 5.05 ± 0.53 | 44.33 ± 9.24 | 2.563 | 2.047 | 3.01 | 0.12 | ||
17 | 10016239 | 4.92 ± 0.38 | 90 ± 12 | 1.13 | |||||
18 | 10162436 | 11.59 ± 0.88 | 47.06 ± 11.72 | 3.303 | 2.267 | 4.91 | 0.15 | ||
19 | 10355856 | 4.47 ± 0.28 | 20.39 ± 3.14 | 124.707 | 70.213 | 3.67 | 0.02 | ||
20 | 10644253 | 10.89 ± 0.81 | 43.44 ± 14.48 | 0.991 | 0.717 | 1.59 | 0.22 | ||
21 | 11070918 | 2.91 ± 0.18 | ... | 2.39 | |||||
22 | 12009504 | 9.48 ± 0.85 | 90 ± 27 | 1.185 | 0.903 | 2.02 | 0.20 | ||
Sun | 26 | 90 | 1.222 | 0.923 | 2.108 | 0.30 |
Notes. Rol and Rog are local and global Rossby numbers computed from tailored models, while Ro(N84) is the Rossby number derived from the B − V colour as in Noyes et al. (1984). The last column contains the depth of the convective zone (as a function of the stellar radius) when available with asteroseismology.
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