Open Access

Table A.1.

Rotational isochrones constructed with our updated two-zone model.

Mass (B − V) Ages (Gyr)
0.10 0.12 0.15 0.20 0.22 0.25 0.30 0.40 0.50 0.60 0.70 1.00 1.50 2.00 2.50 4.00 4.57
0.45 1.477 9.69 9.76 10.94 14.87 15.95 17.10 18.24 19.99 21.54 22.93 24.18 27.21 29.88 31.11 31.90 33.36 34.42
0.50 1.440 9.08 9.27 11.81 14.43 14.99 15.63 16.49 17.80 18.76 19.53 20.18 21.68 23.19 24.66 26.11 30.52 32.41
0.55 1.390 8.40 9.89 11.53 12.43 12.76 13.24 14.00 15.30 16.18 16.69 17.04 17.92 19.47 21.26 23.27 29.82 32.72
0.60 1.338 8.26 9.63 10.38 11.24 11.50 11.84 12.28 12.94 13.43 13.88 14.30 15.61 17.87 20.20 22.62 30.29 33.27
0.65 1.277 8.18 8.60 9.25 9.97 10.16 10.39 10.71 11.22 11.68 12.16 12.61 14.12 16.77 19.62 22.62 31.49 34.70
0.70 1.186 7.38 7.88 8.38 8.83 8.96 9.12 9.38 9.87 10.40 10.92 11.46 13.21 16.30 19.50 22.77 31.96 35.11
0.75 1.072 6.73 7.15 7.51 7.87 7.97 8.12 8.39 8.92 9.49 10.10 10.72 12.69 16.12 19.55 22.86 31.74 34.68
0.80 0.961 6.19 6.42 6.64 6.94 7.06 7.24 7.56 8.19 8.86 9.55 10.25 12.42 16.05 19.49 22.69 31.01 33.76
0.85 0.867 5.65 5.79 5.97 6.29 6.41 6.61 6.95 7.66 8.39 9.14 9.90 12.18 15.85 19.21 22.26 30.01 32.56
0.90 0.787 5.14 5.31 5.50 5.82 5.95 6.15 6.50 7.22 7.96 8.73 9.51 11.82 15.41 18.59 21.46 28.69 31.09
0.95 0.718 4.67 4.81 5.01 5.36 5.51 5.73 6.11 6.87 7.64 8.41 9.19 11.42 14.79 17.75 20.40 27.15 29.38
1.00 0.661 4.33 4.45 4.64 4.98 5.12 5.33 5.70 6.45 7.21 7.95 8.69 10.79 13.91 16.63 19.06 25.23 27.32
1.05 0.609 3.99 4.10 4.29 4.62 4.75 4.96 5.31 5.99 6.69 7.36 8.02 9.91 12.70 15.14 17.31 22.94 24.92
1.10 0.564 3.67 3.78 3.96 4.25 4.36 4.53 4.82 5.40 5.99 6.56 7.12 8.74 11.12 13.19 15.03 20.03 22.02
1.15 0.523 3.35 3.44 3.58 3.81 3.91 4.05 4.28 4.75 5.20 5.63 6.07 7.28 9.11 10.72 12.19 16.67 18.78
1.20 0.484 3.01 3.09 3.21 3.40 3.46 3.55 3.69 3.94 4.19 4.44 4.69 5.45 6.62 7.69 8.74 13.70 ***
1.25 0.448 2.75 2.77 2.78 2.82 2.84 2.86 2.89 2.97 3.05 3.12 3.17 3.35 3.58 3.96 4.69 10.86 ***

Notes. Surface rotation period is reported in days. In the isochrone at 4.57 Gyr, missing entries (indicated by ***) correspond to stars that have already left the main sequence by that age.

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