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Table 1
IRV distributions for massive stars (Limongi & Chieffi 2018 models, set R) tested in this study in addition to the reference set (R150; see Sect. 2.3).
| Model | IRV distribution (% at [Fe/H] = −3, −2, −1, 0) |
|---|---|
| R300 | 300 km s−1: 100, 100, 100, 100 |
| DIS2 (Molero et al. 2024) | 0 km s−1: 10,20, 30, 45 150 km s−1: 10, 30, 50, 50 300 km s−1: 80, 50, 20,5 |
| DIS3 (Romano et al. 2019) | 0 km s−1: 0, 0, 100, 100 300 km s−1: 100, 100, 0, 0 |
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