Table 3
Input parameters for the chemical evolution models represented in Figure 7.
| Model name | Chemical evolution scenario | Yields for AGB | Yields for MS |
|---|---|---|---|
| Model 2 | Three-infall model | FRUITY original | (1) − vrot = 150 km s−1 |
| Model 6 | Three-infall model | FRUITY original | (1) – Distribution from (2) |
| Model 7 | Three-infall model | FRUITY original | (1) – Distribution from (3) |
Notes. The models differ by the yields used for rotating massive stars. In Model 6, the initial rotational velocity of massive stars follows the distribution DIS 3 of (2) (vrot = 150 km s−1 for metallicities Z < 3.236 × 10−3, vrot = 0 km s−1 afterwards). In Model 7, it follows the one presented in (3). Model 2 uses a fixed rotational velocity of vrot = 150 km s−1. See text for more details. (1) Limongi & Chieffi (2018); (2) Molero et al. (2024); (3) Prantzos et al. (2018).
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