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Table 4.

Properties of all the stars at the last computed model, remnant types and masses, and averaged mass fractions of different elements above the remnant mass.

Crit. Mini Mfin log Teff, fin log Lfin Remnant
 1H 4He 12C 16O 𝒵 (†)
(M⊙) (M⊙) (K) (L⊙) Type (M⊙) (mass frac.)
Led. 120 0.4 30.8 5.4 6.2 BH 30.8 0.00 0.11 0.343 0.494 0.049
Sch. 120 0.4 19.0 5.4 5.9 BH 19.0 0.00 0.12 0.395 0.418 0.064
Led. 120 – 28.6 5.3 6.2 BH 28.6 0.00 0.12 0.358 0.469 0.051
Sch. 120 – 30.9 5.3 6.2 BH 30.9 0.00 0.12 0.346 0.469 0.061
Led. 85 0.4 22.7 5.4 6.0 BH 22.7 0.00 0.11 0.374 0.430 0.082
Sch. 85 0.4 26.4 5.4 6.1 BH 26.4 0.00 0.12 0.367 0.451 0.058
Led. 85 – 19.0 5.4 6.0 BH 19.0 0.00 0.12 0.389 0.424 0.066
Sch. 85 – 18.6 5.4 6.0 BH 18.6 0.00 0.12 0.391 0.426 0.065
Led. 60 0.4 16.8 5.4 5.9 BH 16.8 0.00 0.12 0.394 0.428 0.060
Sch. 60 0.4 18.0 5.4 5.9 BH 18.0 0.00 0.12 0.396 0.418 0.064
Led. 60 – 13.9 5.4 5.8 BH 13.9 0.00 0.13 0.411 0.406 0.057
Sch. 60 – 12.5 5.3 5.7 BH 12.5 0.00 0.12 0.413 0.401 0.061
Led. 40 0.4 15.4 5.4 5.8 BH 15.4 0.00 0.10 0.389 0.458 0.051
Sch. 40 0.4 12.3 5.3 5.6 BH 12.3 0.00 0.12 0.411 0.420 0.045
Led. 40 – 12.9 5.3 5.7 BH 12.9 0.00 0.09 0.370 0.478 0.061
Sch. 40 – 13.7 4.6 5.7 BH 13.7 0.00 0.56 0.165 0.204 0.073
Led. 32 0.4 14.0 4.5 5.7 BH 14.0 0.00 0.53 0.207 0.225 0.031
Sch. 32 0.4 10.1 5.3 5.5 BH 10.1 0.00 0.12 0.403 0.441 0.032
Led. 32 – 11.3 4.6 5.6 BH 11.3 0.00 0.58 0.150 0.210 0.058
Sch. 32 – 10.9 4.6 5.6 BH 10.9 0.00 0.71 0.112 0.119 0.058
Led. 25 0.4 10.4 4.3 5.4 BH 10.4 0.02 0.58 0.183 0.188 0.030
Sch. 25 0.4 9.7 4.4 5.5 NS 1.57 0.00 0.20 0.209 0.525 0.070
Led. 25 – 9.3 4.4 5.5 BH 9.3 0.01 0.74 0.106 0.105 0.042
Sch. 25 – 8.3 4.4 5.4 NS 1.55 0.00 0.33 0.171 0.417 0.081
Led. 20 0.4 7.3 3.8 5.3 NS 1.65 0.00 0.30 0.219 0.454 0.028
Sch. 20 0.4 7.2 4.3 5.3 NS 1.65 0.00 0.29 0.165 0.427 0.113
Led. 20 – 7.0 4.0 5.2 NS 1.51 0.01 0.37 0.134 0.351 0.141
Sch. 20 – 8.6 3.6 5.2 NS 1.77 0.17 0.48 0.072 0.174 0.105
Led. 15 0.4 12.4 3.6 5.1 NS 1.55 0.42 0.40 0.047 0.100 0.036
Sch. 15 0.4 11.1 3.6 5.1 BH 11.1 0.39 0.45 0.045 0.094 0.019
Led. 15 – 13.0 3.6 4.9 NS 1.4 0.51 0.36 0.032 0.065 0.037
Sch. 15 – 13.2 3.6 4.9 NS 1.4 0.49 0.41 0.025 0.045 0.033
Led. 12 0.4 11.1 3.6 4.8 NS 1.4 0.49 0.42 0.025 0.051 0.021
Sch. 12 0.4 10.2 3.6 4.9 NS 1.4 0.46 0.38 0.041 0.102 0.026
Led. 12 – 11.1 3.5 4.7 NS 1.4 0.56 0.37 0.018 0.030 0.017
Sch. 12 – 11.3 3.6 4.7 NS 1.4 0.56 0.37 0.016 0.031 0.019
Led. 9 0.4 8.7 3.6 4.3 WD 0.93 0.52 0.39 0.016 0.039 0.031
Sch. 9 0.4 8.5 3.5 4.6 WD 1.18 0.48 0.41 0.024 0.050 0.03
Led. 9 – 8.7 3.6 4.1 WD 0.82 0.58 0.36 0.022 0.026 0.011
Sch. 9 – 8.8 3.6 3.9 WD 0.83 0.58 0.36 0.007 0.020 0.034
Led. 7 0.4 6.9 3.6 3.7 WD 0.60 0.54 0.38 0.026 0.048 0.013
Sch. 7 0.4 6.9 3.6 3.8 WD 0.61 0.54 0.36 0.029 0.058 0.013
Led. 7 – 6.9 3.6 3.8 WD 0.54 0.59 0.35 0.027 0.029 0.011
Sch. 7 – 6.9 3.6 3.5 WD 0.57 0.59 0.33 0.028 0.035 0.014

Notes. We took the stellar properties at the end of core C-burning for the rotating 9 M⊙ models and all models 12 M⊙ and above, at the end of core He-burning for the 7 M⊙ and non-rotating 9 M⊙ models. In the case of direct collapse to a black hole, we give the averaged mass fractions of elements above the mass of the CO core.

(†)

( † )Usually, Z refers to metallicity: Z = 1 − X − Y, where X and Y are the mass fractions of 1H and 4He, respectively. Because we refer to metallicity excluding 12C and 16O, we used the calligraphic 𝒵 = 1 − X − Y − X(12C)−X(16O).

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