Table 6.
Input physics of the stellar models. All sets include models at 0.55, 0.60, 0.65, 0.70, 0.75, and 0.78 M⊙.
| Code | Montréal/Montpellier (a) | CESTAM (b) | ||||||
|---|---|---|---|---|---|---|---|---|
| Model set | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 |
| T0 [106 K] (1) | 1.0, 1.32, 1.74, 1.80, 1.90, 2.24 | 1.60, 1.74, 1.80, 1.90 | – | – | – | – | – | – |
| vZAMS [km.−1] | – | – | 15 | 15 | 15 | 15 | 15 | 15 |
| νv, add [cm2.s−1] | – | – | 108 | 0 | 108 | 108 | 108 | 108 |
| αovi [Hp] | – | – | – | – | 0.1 | 0.3 | 0.4 | 0.6 |
| Opacities | OPAL monochromatic (c) | OP (d) | ||||||
| Eos | CEFF (e) | OPAL2005 (f) | ||||||
| Nuc. react. | Bahcall92 (g) | NACRE+LUNA (h) | ||||||
| αconv. | 1.66 (i) | 0.69 (j) | ||||||
| Initial mix. | AGSS09 (k) | |||||||
| Xini | 0.7538 | |||||||
| Yini | 0.2461 | |||||||
| (7Li/H)×1010 | 4.45 | |||||||
| [Fe/H] | −2.31 | |||||||
| α enhanc. | +0.3 | |||||||
| Core ov. | None | |||||||
Notes. The complete initial chemical composition is available in Deal et al. (2021).
Reference temperature in the expression of Dturb (see Eq. (25)).
Solar calibrated value with the Böhm-Vitense (1958) formalism.
Solar calibrated value with the Canuto et al. (1996) formalism for models including atomic diffusion.
References.
Iglesias & Rogers (1996), tables not public.
Angulo (1999) + Imbriani et al. (2004) for 14N(p, γ)15O.
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