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Table 1

Main ingredients of the evolutionary models.

STERN1 Geneva2 FRANEC3 Padova4 MESA5 STAREVOL5

Initial metallicity (Z) 0.0088 0.0140 0.01345 0.0170 0.014 0.0134
Mixing length parameter (l/HP) 1.5 1.6 / 1.0 2.3 1.68 2.0 1.63
Overshoot parameter (d/HP) 0.335 0.1 0.2 ~0.5 f = 0.0/0.01/0.02 0.0/0.1/0.2
Rotation 0−550 km s-1 Ω/Ωcrit = 0.4 300 km s-1 0 0/200 km s-1 0/220 km s-1
Magnetic field Spruit-Taylor no no no no no
Solar mixture AGS056 AGS05 AGSS097 GN938 GN93 AGSS09
with C, N, O, with Ne enhanced
Mg, Si, Fe modified (Cunha et al. 2006)

Reference. 1) Brott et al. (2011a); 2) Ekström et al. (2012); 3) Chieffi & Limongi (2013); 4) Bertelli et al. (2009); 5) this work. Heavy elements solar mixture: 6) Asplund et al. (2005); 7) Asplund et al. (2009); 8) Grevesse et al. (1993). For stars with initial mass <40 M, the mixing length parameter is l/HP = 1.6. For more massive stars, it is defined with respect to the local density scale height and l/Hρ = 1.0. In MESA the overshooting is implemented as a decreasing exponential with parameter f (see text).

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