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Table 2.
Modified nucleosynthesis yields.
| Prescriptions of NEW MW and NEW LMC models | |||
|---|---|---|---|
| Element | LIMS | Massive stars | SNIa |
| (Karakas 2010) | (Kobayashi et al. 2006) | (Iwamoto et al. 1999) | |
| Fe | ✓ | ×0.7 | ✓ |
| Mg | ✓ | Z ∈ (3 − 8)×10−3 → ×1.2 | ✓ |
| Z > 8 × 10−3 → ×(Z/0.004)0.4 | |||
| Al | Z > 8 × 10−3 → ×0.8 | ×1.5 | ✓ |
| Mn | ✓ | ✓ | ×(Z/Z⊙)0.65 (from Cescutti et al. 2008) |
Notes. Correction factors adopted in the NEW MW and NEW LMC models for Fe, Mg, Al, and Mn considering the same stellar sources as in Vasini et al. (2022, 2023). These same prescriptions were also used in the WIND MW model.
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