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Table 5

Characteristics of stellar evolution models with rotation.

mass Teff log g L vsurf ALi Age Phase
(M⊙) (K) (dex) (L⊙) (km s-1) (dex) (Gyr)
KK = 0 KK ≠ 0 KK = 0 KK ≠ 0 KK = 0 KK ≠ 0 KK = 0 KK ≠ 0 KK = 0 KK ≠ 0 KK = 0 KK ≠ 0
1.30 6699 6701 4.37 4.37 2.75 2.75 12.05 18.9 3.18 3.18 4.48 × 10-2 4.76 × 10-2 ZAMS
6439 6440 3.99 3.99 5.55 5.57 10.86 8.88 2.99 1.26 3.36 3.38 TO
6212 6218 3.89 3.89 6.11 6.15 7.97 8.03 2.93 1.14 3.7 3.7 M 67
1.31 6729 6729 4.36 4.36 2.85 2.85 11.92 18.87 3.18 3.18 4.50 × 10-2 4.50 × 10-2 ZAMS
6457 6472 3.99 3.99 5.70 5.70 10.72 9.00 2.93 1.27 3.24 3.24 TO
6050 6056 3.82 3.82 6.48 6.49 7.40 7.22 2.80 1.08 3.7 3.7 M 67
1.32 6757 6758 4.36 4.36 2.95 2.96 11.88 18.90 3.18 3.18 4.26 × 10-2 4.26 × 10-2 ZAMS
6476 6499 3.99 4.00 5.88 5.79 10.75 9.05 2.93 1.23 3.19 3.11 TO
5824 5724 3.77 3.75 6.38 6.20 5.84 5.73 2.65 0.93 3.7 3.7 M 67
1.33 6787 6787 4.36 4.36 3.06 3.06 12.09 18.92 3.17 3.18 3.88 × 10-2 4.02 × 10-2 ZAMS
6479 6508 3.97 3.99 6.11 6.05 10.71 9.15 2.92 1.32 3.14 3.07 TO
5266 5211 3.70 3.68 4.98 4.89 3.63 4.14 1.82 0.19 3.7 3.7 M 67
1.34 6814 6808 4.35 4.35 3.16 3.17 12.09 18.97 3.17 3.17 3.66 × 10-2 3.78 × 10-2 ZAMS
6502 6526 3.97 3.98 6.28 6.22 10.71 9.24 2.93 1.37 3.05 2.99 TO
5010 4978 3.54 3.49 5.88 6.59 2.54 3.08 1.44 –0.15 3.7 3.7 M 67
1.35 6841 6842 4.35 4.35 3.28 3.28 12.09 18.97 3.17 3.18 3.38 × 10-2 3.56 × 10-2 ZAMS
6552 6544 3.98 3.98 6.43 6.41 10.90 9.33 2.93 1.38 2.94 2.91 TO
4909 4940 3.29 3.37 9.86 8.35 1.88 2.73 1.30 –0.23 3.7 3.7 M 67
1.36 6875 6877 4.34 4.34 3.34 3.34 12.23 19.33 3.17 3.17 2.95 × 10-2 3.02 × 10-2 ZAMS
6559 6521 3.97 3.95 6.63 6.74 10.81 9.33 2.94 1.37 2.84 2.91 TO
4709 4752 2.78 3.02 26.90 22.87 1.11 1.60 1.26 –0.37 3.7 3.7 M 67
1.37 6898 6902 4.34 4.34 3.51 3.51 12.23 20.45 3.17 3.17 3.03 × 10-2 2.98 × 10-2 ZAMS
6515 6555 3.94 3.95 6.95 6.88 10.40 9.87 2.93 1.15 2.88 2.82 TO
4637 4453 2.61 2.23 37.87 76.04 0.94 0.91 1.03 –0.61 3.7 3.7 M 67

Notes. Effective temperature, surface gravity, luminosity, surface rotation velocity, lithium abundance, age, and associated evolutionary phase are given for models with initial masses between 1.30 M⊙ and 1.37 M⊙. In the last column, “M 67” refers to the models predictions at the adopted age for the cluster of 3.7 Gyr. For each quantity, the values for models without (KK = 0) and with (KK ≠ 0) magnetic braking on the ZAMS are indicated.

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