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Table 6

Grids of dedicated stellar evolution models computed from the pre-main sequence (PMS) to the early-AGB stage.

Type υZAMS M Z [C/Fe]ini [N/Fe]ini [O/Fe]ini [Na/Fe]ini Mixing
km s-1 (M) (dex) (dex) (dex) (dex)

S 0 3.0–5.5 0.012294 0 0 0 0 overshoot αov = 0.1Hp
SlZ 0 3.0–5.5 0.0070188 0 0 0 0 overshoot αov = 0.1Hp
CNO 0 3.0–5.5 0.025824 1.218 1.295 0.238 0.370 overshoot αov = 0.1Hp
RotCNO 25 3.5; 3.8 0.0070188 1.218 1.295 0.238 0.370 overshoot αov = 0.1Hp
rot. mix. Maeder & Zahn (1998)
SlowRot 25 3.0–5.5 0.012294 0 0 0 0 overshoot αov = 0.1Hp
rot. mix. Maeder & Zahn (1998)
FastRot 180 3.0; 3.5 0.012294 0 0 0 0 overshoot αov = 0.1Hp
rot. mix. Maeder & Zahn (1998)

Notes. All models are computed using Asplund et al. (2005) as a reference for the solar abundances mixture (Z = 0.012294).

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