Table B.1.
Carbon, nitrogen, and oxygen initial abundances of the models considered.
| Ekström et al. (2012) | Eggenberger et al. (2021) | Keszthelyi et al. (2022) | Jin et al. (in prep.) | |
|---|---|---|---|---|
| ϵC, i [XC, i/10−3] | 8.39 [2.31] | 8.01 [0.99] | 8.33 [1.85] | 8.52 [2.85] |
| ϵN, i [XN, i/10−3] | 7.78 [0.66] | 7.40 [0.28] | 7.79 [0.62] | 7.88 [0.77] |
| ϵO, i [XO, i/10−3] | 8.66 [5.73] | 8.28 [2.46] | 8.76 [6.63] | 8.74 [6.39] |
| XCNO, i/10−3 | 8.7 | 3.73 | 9.1 | 10.01 |
Notes. Initial C, N, and O abundances assumed in the SSEM considered in this work. Individual C, N, O abundances in the usual ϵX = log(N(X)/N(H)) + 12 scale, and in brackets in mass fraction. Total CNO (XCNO, i) abundances in mass fraction. In Eggenberger et al., initial abundances of elements different than H and He were scaled with metallicity (see text).
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