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Table 1.

Variable input parameters of the PoWR models along the evolutionary tracks of the nonrotating 150 M models.

Grid t M log(L/L) Rshallow Rdeep log ( M ˙ $ \log(\dot{M} $/ v H C N O Ne
point Myr /M /R /R M yr) /km s−1 /10−4 /10−4 /10−4 /10−3
00 0.02 149.7 6.382 17.23 15.69 −4.831 4795 0.7200 23.11 6.588 57.34 2.029
01 0.34 144.7 6.383 19.01 16.90 −4.769 4481 0.7200 23.11 6.588 57.34 2.029
02 0.61 139.6 6.384 20.41 17.67 −4.701 4243 0.7200 23.11 6.588 57.34 2.029
03 0.85 134.6 6.386 22.16 18.49 −4.630 3992 0.7198 13.17 18.49 57.22 2.028
04 1.04 129.7 6.387 23.37 18.94 −4.583 3810 0.7016 0.7560 60.49 25.54 1.894
05 1.23 124.7 6.388 24.39 19.16 −4.545 3652 0.6702 0.9214 74.19 9.662 1.867
06 1.40 119.5 6.390 25.36 19.24 −4.513 3499 0.6322 0.9863 79.19 3.873 1.858
07 1.56 114.6 6.392 26.40 19.27 −4.484 3354 0.5917 1.013 80.80 1.990 1.850
08 1.70 109.7 6.393 27.50 19.21 −4.458 3207 0.5481 1.028 81.31 1.386 1.841
09 1.84 104.5 6.395 28.77 19.02 −4.431 3053 0.4993 1.041 81.46 1.197 1.832
10 1.97 99.7 6.397 30.03 18.74 −4.409 2909 0.4513 1.055 81.50 1.142 1.823
11 2.10 94.7 6.399 31.85 18.39 −4.384 2741 0.3994 1.066 81.50 1.117 1.812
12 2.22 89.4 6.401 33.91 17.84 −4.360 2563 0.3417 1.086 81.50 1.096 1.801
13 2.33 84.6 6.404 36.42 17.23 −4.338 2395 0.2889 1.103 81.50 1.076 1.791
14 2.43 79.6 6.407 39.43 16.31 −4.310 2209 0.2315 1.127 81.49 1.052 1.780
15 2.53 74.7 6.414 36.04 13.54 −4.266 2216 0.1740 1.156 81.48 1.022 1.769

Notes. The abundances in the last five columns are given as mass fractions.

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