Table A.2.
MESA stellar models with 40% critical initial rotation.
| Z | MZAMS | Vrot, i | MHe | MCO, 1 | MCO, 2 | PNS, aspin | MNS/BH | Mstar, m | Mstar, st1 | Mstar, st2 |
|---|---|---|---|---|---|---|---|---|---|---|
| [M⊙] | [km s−1] | [M⊙] | [M⊙] | [M⊙] | [ms] | [M⊙] | [M⊙] | [M⊙] | [M⊙] | |
| Z = 0.014 | 10 | 257 | 2.9 | 1.2 | 1.5 | 8.0 | 1.20 | 3.4 | 9.4 | 9.8 |
| 15 | 270 | 4.5 | 2.2 | 2.7 | 6.4 | 1.27 | 5.7 | 11.3 | 13.9 | |
| 20 | 274 | 6.7 | 3.6 | 4.6 | 4.4 | 1.79 | 10.8 | 12.3 | 17.6 | |
| 25 | 276 | 7.8 | 4.2 | 6.2 | 0.094 | 6.16 | 19.9 | 9.2 | 20.4 | |
| 32 | 272 | 12.0 | 7.9 | 9.1 | 0.107 | 9.23 | 25.3 | 10.5 | 23.4 | |
| 40 | 267 | 16.6 | 11.8 | 13.2 | 0.105 | 16.8 | 27.8 | 11.6 | 22.1 | |
| 60 | 254 | 27.6 | 21.1 | 22.6 | 0.083 | 28.0 | 46.5 | 13.5 | 36.0 | |
| 85 | 239 | 41.6 | 33.4 | 35.2 | 0.046 | 42.6 | 56.2 | 18.1 | 52.6 | |
| 120 | 220 | 60.8 | 49.9 | 52.8 | 0.037 | 55.0 | 80.0 | 20.7 | 66.9 | |
| Z = 0.006 | 10 | 268 | 2.9 | 1.0 | 1.6 | 6.7 | 1.20 | 3.9 | 9.6 | 9.9 |
| 15 | 279 | 4.7 | 2.2 | 2.9 | 5.9 | 1.32 | 10.0 | 13.5 | 14.5 | |
| 20 | 293 | 6.8 | 3.8 | 4.6 | 9.7 | 1.79 | 18.3 | 16.7 | 19.0 | |
| 25 | 296 | 8.6 | 5.1 | 6.0 | 0.101 | 8.67 | 23.0 | 17.8 | 22.8 | |
| 32 | 295 | 11.8 | 7.9 | 8.9 | 0.100 | 8.87 | 29.3 | 17.5 | 27.5 | |
| 40 | 289 | 14.4 | 8.9 | 10.3 | 0.099 | 16.1 | 31.3 | 14.8 | 21.3 | |
| 60 | 277 | 26.6 | 20.3 | 21.9 | 0.093 | 26.8 | 52.4 | 18.9 | 38.6 | |
| 85 | 266 | 39.9 | 31.2 | 32.9 | 0.081 | 47.1 | 69.0 | 28.8 | 61.5 | |
| 120 | 251 | 61.8 | 50.6 | 53.3 | 0.072 | 55.0 | 91.7 | 31.4 | 77.9 | |
| Z = 0.002 | 10 | 285 | 3.0 | 1.1 | 1.6 | 7.1 | 1.20 | 6.5 | 8.4 | 9.6 |
| 15 | 298 | 4.9 | 2.5 | 3.0 | 7.7 | 1.35 | 14.7 | 12.8 | 14.6 | |
| 20 | 305 | 6.6 | 3.7 | 4.3 | 7.6 | 1.72 | 19.5 | 17.8 | 19.3 | |
| 25 | 310 | 8.2 | 4.9 | 7.7 | 0.096 | 8.29 | 23.9 | 19.8 | 23.4 | |
| 32 | 312 | 12.0 | 8.1 | 9.0 | 0.104 | 9.11 | 30.4 | 18.9 | 28.0 | |
| 40 | 313 | 15.4 | 10.9 | 12.1 | 0.142 | 15.4 | 37.3 | 14.5 | 17.1 | |
| 60 | 304 | 26.9 | 20.8 | 22.4 | 0.108 | 27.0 | 55.1 | 22.8 | 39.3 | |
| 85 | 286 | 39.5 | 31.6 | 33.6 | 0.090 | 39.7 | 76.9 | 35.7 | 66.6 | |
| 120 | 268 | 60.9 | 50.1 | 54.1 | 0.065 | 55.0 | 105 | 46.6 | 91.6 | |
| Z = 0.0004 | 10 | 302 | 3.1 | 1.4 | 1.7 | 7.1 | 1.20 | 9.8 | 9.9 | 10.0 |
| 15 | 315 | 4.9 | 2.5 | 3.1 | 8.5 | 1.36 | 14.9 | 14.8 | 14.9 | |
| 20 | 323 | 6.8 | 3.9 | 4.6 | 5.2 | 1.79 | 19.7 | 19.7 | 19.9 | |
| 25 | 329 | 8.7 | 5.4 | 6.2 | 0.138 | 8.81 | 24.5 | 24.4 | 24.8 | |
| 32 | 335 | 12.4 | 8.3 | 9.3 | 0.110 | 9.83 | 31.0 | 30.0 | 31.4 | |
| 40 | 338 | 14.3 | 9.7 | 10.7 | 0.109 | 13.7 | 38.3 | 15.6 | 23.4 | |
| 60 | 341 | 40.0 | 32.3 | 34.1 | 0.058 | 43.1 | 55.7 | 24.9 | 41.7 | |
| 85 | 340 | 43.3 | 34.7 | 36.9 | 0.097 | 41.7 | 79.9 | 37.9 | 68.5 | |
| 120 | 334 | 63.1 | 47.3 | 61.1 | 0.072 | 28.4 | 112 | 66.6 | 104 | |
Notes. For all models we list: Z: metallicity, MZAMS: initial star mass, Vrot, i: initial rotation at equator, MHe: He core mass, MCO, 1: CO core mass defined by < 1% He (used in MESA), MCO, 2: CO core mass defined by > 20% CO (adopted in our study), PNS, aspin: for NSs, the NS spin period in milliseconds, for BHs, the dimensionless spin magnitude, MNS/BH: remnant mass, Mstar, m: final mass of a star in MESA, Mstar, st1: final mass of a star in StarTrack with standard winds, Mstar, st2: final mass of a star in StarTrack with reduced (30%) winds.
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