Open Access
Table 1.
Main components of our grid of stellar models.
| Parameter | Range |
|---|---|
| Initial mass in M⊙ | [0.7–1.6], ΔM = 0.05 |
| Initial metallicity in dex | [−0.5–0.5], Δ[Fe/H] = 0.1 |
| Enrichment ratio, ΔY/ΔZ | [0.4–2.4], Δ(ΔY/ΔZ) = 0.4 |
| Input physics | Prescription |
| Nuclear reaction rates | 1, 2 |
| Solar chemical mixtures | 3 |
| OPAL equation of state | 4 |
| OPAL opacities | 5, 6 |
| Atmosphere model | 7 |
| Atomic diffusion | 8 |
| Core overshooting, fov = 0.01 | 9 |
| αMLT = 1.71 | 10 |
Notes. (1) Angulo et al. (1999); (2) Imbriani et al. (2005); (3) Asplund et al. (2009); (4) Rogers & Nayfonov (2002); (5) Iglesias & Rogers (1996); (6) Ferguson et al. (2005); (7) Krishna Swamy (1966); (8) Thoul et al. (1994); (9) Herwig (2000); (10) Cox & Giuli (1968).
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