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Table 2.

Stellar yields of nitrogen and oxygen for different Pop III and very metal-poor stellar models.

Mini MCO Mrem Final 14N 16O
[M] [M] [M] fate [M] [M]
Z = 0
υini = 0
9 0.718 0.718 WD 2.52E−08 0.109
20 4.047 1.517 NS 1.39E−03 1.719
60 22.575 26.575 BH 1.01E−04 4.42E−07
85 31.768 35.768 BH 2.26E−05 0.008
120 52.887 34.640 PPISN 9.02E−06 15.969
υini = 0.2 υcrit
9 0.940 0.940 WD 2.89E−05 0.173
12 1.385 1.385 WD 1.27E−04 0.173
15 2.180 1.400 NS 2.88E−04 0.814
20 ( * ) 19.99 19.99 BH 0.0 0.0
υini = 0.4 υcrit
9 0.895 0.895 WD 0.0011 0.304
20 3.981 1.785 NS 2.26E−07 2.006
60 ( * ) 19.373 23.373 BH 8.54E−07 1.06E−08
85 ( * ) 30.465 34.465 BH 7.15E−06 2.07E−06
120 ( * ) 56.397 30.550 PPISN 0.0007 16.540
υini = 0.7 υcrit
9 1.389 1.389 WD 0.004 0.551
20 8.679 12.679 BH 0.207 0.213
60 14.442 18.442 BH 3.760 0.914
85 33.07 37.070 BH 0.706 3.068
120 ( * ) 61.645 0.0 PISN 0.318 26.707

Z = 10−5

υini = 0
9 1.009 1.009 WD 1.91E−05 0.123
20 3.748 7.748 BH 3.79E−05 −8.67E−05
60 20.925 24.925 BH 1.70E−04 −9.96E−05
85 31.622 35.622 BH 2.51E−04 0.001
120 47.977 41.620 PPISN 2.66E−04 6.292
υini = 0.4 υcrit
9 1.119 1.119 WD 0.008 0.529
20 2.980 6.980 BH 0.171 0.216
60 13.419 17.419 BH 2.902 1.750
85 37.358 41.358 BH 0.051 0.652
120 59.437 0.0 PISN 0.012 53.17

Notes. The asterisk after the initial mass indicates that the model is still in the core He-burning phase. The Pop III models with υini/υcrit = 0, 0.2, and 0.4 are from Murphy et al. (2021a) and the models with Z = 10−5 are from Sibony et al. (in prep.).

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