Table 1.
List of stellar evolutionary model grids
| Grid | B | S | CC-S | CC-He |
|---|---|---|---|---|
| System | Binary | Single | Single | Single HeS |
| Mi or M1, i [ M⊙] | 5 − 100 | 5 − 12.6 | 12.6 − 200 | 2.5 − 40.7 |
| Pi [ d] | 1.3 − 5011 | – | – | – |
| qi | 0.10 − 0.95 | – | – | – |
| vrot, i | 0.2 vcrit | 150 km s−1 | 0.2 vcrit | No |
| Network | stern | approx21 | ||
| Termination | core C depletion | core-collapse | ||
| Reference | [1] | [2] | This work | |
Notes. The first row shows the acronym with which we refer to each grid. Each row then shows whether they evolve as a binary-star system, a single-star system or a single helium star (HeS) system (2), the initial mass of the stellar model or of the initially more massive star if it is in a binary system (3), initial orbital period and mass ratio (4–5), rotation (6), the nuclear network adopted (7), the latest evolutionary phase that can be captured by these models (8), and the reference (9). References: [1] Jin et al. 2025, [2] Jin et al. 2024.
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