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Table 1.

Properties of Pop III models at the end of the core H- and He-burning phases with different initial surface velocities.

End MS End He-burning
Mini υsurf τH υ/υcrit υsurf Ysurf τHe υ/υcrit υsurf Ysurf
[M] [km s−1] [Myrs] [km s−1] [Myrs] [km s−1]
υini = 0
9 0 17.7 0 0 0.248 1.9 0 0 0.248
20 0 9.5 0 0 0.248 0.6 0 0 0.248
60 0 3.7 0 0 0.248 0.3 0 0 0.248
85 0 3.1 0 0 0.248 0.3 0 0 0.248
120 0 2.7 0 0 0.248 0.3 0 0 0.248
υini = 0.2 υcrit
9 23.1 19.9 0.18 124 0.255 3.3 0.10 41 0.260
12 27.6 19.4 0.18 125 0.258 1.3 0.09 25 0.260
15 31.5 14.3 0.19 134 0.258 0.01 0.09 22 0.259
20 37.2 10.4 0.18 128 0.255
υini = 0.4 υcrit
9 372 20.9 0.38 274 0.286 2.5 0.11 60 0.286
20 526 10.7 0.41 309 0.277 1.0 0.44 192 0.277
60 613 4.1 0.87 657 0.265 0.4 0.72 302 0.269
85 659 3.3 0.70 551 0.265
120 708 2.9 0.64 473 0.303
υini = 0.7 υcrit
9 649 26.6 0.71 514 0.370 2.8 0.17 19 0.405
20 833 11.4 0.87 628 0.314 3.0 0.11 7 0.552
60 1080 4.3 0.82 565 0.313 0.3 0.10 12 0.557
85 1150 3.6 1.00 645 0.349 0.3 0.03 3 0.596
120 1230 3.0 0.86 512 0.366

Notes. Models with υini/υcrit = 0, 0.2, and 0.4 are from Murphy et al. (2021a). Models that have not finished the core He-burning phase are indicated with a horizontal dash.

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