Table 2.
Quantities required to estimate the (O/p) ratio corresponding to the oxygen to p-nuclide yield ratio normalized to the solar abundances (Eq. (6)).
| Model label | Mini | υini/υcrit | 17O(α,γ)21Ne | MCO | Mp | 𝒴O | F0 | F1 | np | (O/p)0 | (O/p)1 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [M⊙] | [M⊙] | [M⊙] | [M⊙] | ||||||||
| M25Zm3V0 | 25 | 0 | Best et al. (2013) | 5.90 | 2.37 | 2.75 | 30.2 | 50.8 | 20 | 62.0 | 37.1 |
| M25Zm3V4 | 25 | 0.4 | Best et al. (2013) | 7.61 | 2.93 | 4.56 | 312 | 908 | 10 | 7.30 | 2.50 |
| M25Zm3V7 | 25 | 0.7 | Best et al. (2013) | 7.56 | 2.93 | 5.30 | 1229 | 1814 | 23 | 2.13 | 1.39 |
| ⟨M25Zm3⟩ | − | − | Best et al. (2013) | 7.35 | 2.93 | 4.61 | 649 | 952 | 23 | 3.55 | 2.41 |
| M25Zm3V0B | 25 | 0 | Best et al. (2013)/10 | 5.88 | 2.37 | 2.91 | 62.3 | 154 | 13 | 30.0 | 11.8 |
| M25Zm3V4B | 25 | 0.4 | Best et al. (2013)/10 | 7.64 | 2.93 | 5.23 | 1047 | 1544 | 23 | 2.49 | 1.69 |
| M25Zm3V7B | 25 | 0.7 | Best et al. (2013)/10 | 7.62 | 2.93 | 5.27 | 8373 | 11346 | 25 | 0.31 | 0.23 |
| ⟨M25Zm3B⟩ | − | − | Best et al. (2013)/10 | 7.39 | 2.93 | 4.92 | 3914 | 4963 | 27 | 0.63 | 0.49 |
| M25Zm3V0C | 25 | 0 | Taggart et al. (2019) | 5.88 | 2.37 | 2.91 | 86.3 | 271 | 10 | 21.4 | 6.68 |
| M25Zm3V4C | 25 | 0.4 | Taggart et al. (2019) | 7.65 | 2.93 | 5.21 | 2353 | 3346 | 24 | 1.10 | 0.78 |
| M25Zm3V7C | 25 | 0.7 | Taggart et al. (2019) | 7.57 | 2.93 | 5.28 | 15008 | 21084 | 24 | 0.18 | 0.12 |
| ⟨M25Zm3C⟩ | − | − | Taggart et al. (2019) | 7.37 | 2.93 | 4.91 | 7229 | 9734 | 25 | 0.34 | 0.25 |
Notes. MCO (Col. 5) is the mass of the carbon-oxygen core (or helium-free core), Mp (Col. 6) is the mass of the layers undergoing p-process nucleosynthesis during the explosion, 𝒴O (Col. 7) is the yield (total ejected mass) of oxygen, F0 (Col. 8) is the average overproduction factor (Eq. (2)), F1 (Col. 9) is like F0, but the sum runs only over the np (Col. 10) most abundant p-nuclides, (O/p)0 (Col. 11) and (O/p)1 (Col. 12) are computed with F0 and F1, respectively. The ⟨M25Zm3⟩, ⟨M25Zm3B⟩, and ⟨M25Zm3C⟩ rows correspond to the velocity-averaged yield of the three models above (cf. Sect. 3.6 for details).
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