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Table B.1

Summary of important stellar characteristics.

M i v rot,i τ MS log Li/L⊙ T eff,i M conv,i M over,i M conv,0.2 M over,0.2 M f v rot,f Y s,f Y c,f log Lf/L⊙ T eff,f j
M ⊙ km s-1 Myr K M ⊙ M ⊙ M ⊙ M ⊙ M ⊙ km s-1 K 1015 cm2/s
60 0 3.373 5.704 50 000 42.6 – 30.7 – 43 0 0.393 0.995 6.022 6600 0
60 220 3.407 5.701 49 500 43.8 – 30.7 – 42 0 0.398 0.995 6.023 8800 89
60 273 3.464 5.699 49 200 43.6 – 30.8 – 42 0 0.384 0.995 6.023 5600 89
60 326 3.619 5.698 48 900 43.5 3.0 32.4 2.6 45 1 0.418 0.995 6.056 14 200 85
60 379 3.676 5.694 48 600 43.4 3.1 32.7 2.6 45 1 0.412 0.995 6.061 14 800 84
60 432 4.038 5.691 48 300 43.3 3.1 38.6 2.1 45 518 0.677 0.995 6.133 38 900 237
60 532 4.167 5.684 47 600 43.0 3.2 40.4 1.6 38 383 0.865 0.995 6.098 69 600 212
100 0 2.648 6.102 54 100 80.6 3.8 57.2 3.8 68 0 0.636 0.993 6.336 17 600 0
100 217 2.692 6.099 53 700 82.1 3.6 57.4 3.7 66 1 0.674 0.991 6.331 22 200 98
100 271 2.740 6.098 53 500 81.9 3.5 58.2 3.7 65 12 0.722 0.993 6.337 27 800 97
100 323 2.817 6.096 53 200 81.7 4.3 60.1 3.5 67 7 0.720 0.993 6.354 26 400 105
100 375 2.973 6.094 53 000 81.6 3.5 66.3 2.6 61 64 0.929 0.991 6.345 47 700 130
100 426 3.016 6.093 52 700 81.4 3.5 66.3 2.2 50 39 0.974 0.993 6.236 58 900 88
100 524 3.065 6.088 52 100 81.0 3.7 66.1 1.8 46 64 0.975 0.995 6.213 73 000 83
150 0 2.313 6.382 56 000 131.6 3.7 91.3 4.4 94 0 0.839 0.975 6.553 30 200 0
150 216 2.339 6.381 55 600 131.3 4.1 91.5 4.4 94 4 0.836 0.973 6.553 30 200 121
150 268 2.417 6.380 55 400 131.1 3.7 95.4 4.2 99 11 0.821 0.966 6.573 28 900 144
150 320 2.465 6.378 55 200 130.9 3.8 97.9 3.5 91 17 0.931 0.966 6.550 41 100 139
150 371 2.544 6.377 55 000 130.7 3.9 98.0 2.3 57 15 0.978 0.991 6.313 55 000 47
150 421 2.557 6.376 54 700 130.6 3.8 96.8 2.1 55 17 0.979 0.993 6.300 56 400 48
150 514 2.579 6.372 54 200 130.2 3.9 95.3 2.1 55 17 0.977 0.991 6.293 55 600 51
200 0 2.140 6.567 56 200 181.5 3.9 126.1 4.7 131 0 0.809 0.916 6.698 30 700 0
200 214 2.155 6.566 55 800 181.1 4.0 125.4 4.7 126 9 0.843 0.927 6.693 32 300 159
200 267 2.185 6.565 55 600 180.9 3.9 126.7 5.6 133 8 0.792 0.912 6.700 30 300 190
200 318 2.255 6.564 55 400 180.7 4.0 130.2 3.8 70 2 0.986 0.995 6.436 51 100 37
200 367 2.291 6.563 55 300 180.6 3.9 129.1 2.8 64 3 0.985 0.995 6.383 53 800 37
200 415 2.302 6.562 55 100 180.4 4.1 127.6 2.3 65 2 0.980 0.991 6.387 50 900 41
200 502 2.334 6.560 54 700 179.8 4.1 121.7 2.1 62 6 0.979 0.991 6.362 52 400 43
300 0 1.979 6.811 54 500 281.1 4.7 195.3 4.7 82 0 0.988 0.993 6.519 46 800 0
300 213 2.003 6.810 54 300 280.6 3.8 193.4 4.9 80 1 0.988 0.993 6.509 47 300 17

Notes. From left to right: mass and surface rotational velocity at the ZAMS (index i); main-sequence lifetime; luminosity and effective temperature at the ZAMS; mass of the convective core and the overshoot zone at the first calculated model after the ZAMS and when hydrogen in the core drops below 0.2; mass, surface rotational velocity, helium mass fraction at the surface and in the core, luminosity, effective temperature; and surface specific angular momentum at the end of the main sequence evolution (index f). Several stellar evolution models have not been calculated until the TAMS. In these cases, the main sequence lifetime is extrapolated until the exhaustion of hydrogen in the core and the final values in Cols. 6–16 correspond to the last calculated values. Dashes in the table indicate data which is not available.

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