Table A.1.
26Al wind yields (calculated using Eq. 2) in M⊙ units. The VMS models at Z = 0.006 and Z = 0.014 are from Martinet et al. (in prep.) probing initial masses of 180, 250 and 300 M⊙, while the models at Z = 0.020 are from Yusof et al. (2022), with VMS models computed only for 150 and 300 M⊙. More details on the massive stars models at Z = 0.006 can be found in Eggenberger et al. (2021) and in Ekström et al. (2012) for the ones at Z = 0.014. Dashes indicate where the models where not computed.
| Z = 0.006 | Z = 0.014 | Z = 0.020 | ||||
|---|---|---|---|---|---|---|
| Mass | Non-rotating | V/Vc = 0.4 | Non-rotating | V/Vc = 0.4 | Non-rotating | V/Vc = 0.4 |
| 12 M⊙ | 4.63E-13 | 3.85E-11 | 1.01E-09 | 4.62E-09 | 2.09E-09 | 1.46E-08 |
| 15 M⊙ | 1.94E-12 | 7.73E-10 | 1.48E-10 | 3.09E-08 | 1.12E-09 | 1.00E-07 |
| 20 M⊙ | 1.12E-09 | 4.87E-07 | 5.57E-07 | 4.46E-06 | 1.32E-06 | 5.42E-06 |
| 25 M⊙ | 1.89E-06 | 1.06E-05 | 9.50E-06 | 9.67E-06 | 1.09E-05 | 2.02E-05 |
| 32 M⊙ | 1.67E-05 | 1.24E-05 | 2.04E-05 | 3.08E-05 | 2.72E-05 | 4.25E-05 |
| 40 M⊙ | 2.32E-05 | 1.53E-05 | 3.82E-05 | 3.66E-05 | 4.03E-05 | 6.73E-05 |
| 60 M⊙ | 7.70E-05 | 2.24E-05 | 5.33E-05 | 1.05E-04 | 1.12E-04 | 2.27E-04 |
| 85 M⊙ | 4.25E-05 | 5.17E-05 | 1.67E-04 | 3.21E-04 | 2.78E-04 | 5.68E-04 |
| 120 M⊙ | 9.57E-05 | 1.39E-04 | 3.64E-04 | 7.09E-04 | 6.50E-04 | 1.26E-03 |
| 150 M⊙ | - | - | - | - | 1.17E-03 | 1.96E-03 |
| 180 M⊙ | 1.70E-04 | 3.37E-04 | 8.37E-04 | 1.30E-03 | - | - |
| 250 M⊙ | 3.67E-04 | 6.51E-04 | 1.93E-03 | 2.63E-03 | - | - |
| 300 M⊙ | 5.39E-04 | 8.97E-04 | 3.03E-03 | 3.71E-03 | 5.78E-03 | 6.43E-03 |
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