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Table 1

Properties of the different models computed without rotation (std), with rotation but without IGW (rot), and with rotation taking into account IGW (igw).

Star τ(pms) τ(core) v surf Ωsurf / Ω Pinit v surf Ωsurf P ZAMS N(Li) T eff log L/L
M Myr Myr init, km s-1 init days zams, km s-1 zams days zams zams, K zams

0.6 std 191 7.47 –4.96 4118 –1.14
rot 194 7.47 14.5 6.60 3.73 36.3 34.5 7.30 –5.08 4127 –1.14
igw 217 7.47 14.5 6.60 3.73 37.3 35.6 7.12 –5.40 4121 –1.14

0.9 std 75 3.00 2.66 5246 –0.366
rot 76 3.00 14.1 4.16 5.99 48.5 30.7 0.83 2.64 5246 –0.366
igw 89 3.00 14.1 4.16 5.99 55.7 35.2 0.72 2.64 5246 –0.366

1.0 std 57.5 2.43 2.96 5608 –0.152
rot 53.9 2.43 14.2 3.76 6.84 53.1 29.8 0.76 3.02 5608 –0.152
rot+hydro 59.4 2.43 14.2 3.76 6.84 52.9 29.7 0.76 3.12 5589 –0.152
igw 59.5 2.43 14.2 3.76 6.84 63.1 35.5 0.68 2.95 5608 –0.152
igw+hydro 59.2 2.43 14.2 3.76 6.84 63.1 35.3 0.72 2.95 5584 –0.156

1.2 std 38.6 1.58 3.17 6217 0.235
igw 43.5 1.58 17.2 2.99 8.03 86.7 38.6 0.86 3.17 6217 0.235

1.4 std 26.5 1.09 3.22 6828 0.574
igw 29.4 1.09 13.6 4.08 6.02 109 39.9 0.64 3.22 6838 0.572

1.6 std 19.6 0.81 3.23 7757 0.835
rot 19.3 0.81 13.0 1.85 13.7 100 39.2 0.71 3.23 7757 0.837
igw 21.2 0.81 13.0 1.85 13.7 120 42.2 0.57 3.23 7783 0.829

1.8 std 15.0 0.62 3.24 8666 1.04
rot 15.0 0.62 12.4 1.43 16.9 112 37.6 0.68 3.24 8666 1.04
igw 16.1 0.62 12.4 1.43 16.9 128 43.9 0.57 3.24 8676 1.04

2.0 std 11.8 0.48 3.24 9479 1.23
rot 11.7 0.48 20 3.32 7.62 124 40.7 0.62 3.24 9473 1.23
igw 12.1 0.48 20 3.32 7.62 139 46.0 0.54 3.24 9492 1.23

Notes.For the 1.0 M star a couple of models were computed taking into account the hydrostatic effects of rotation (rot+hydro and igw+hydro). For each model we give: lifetime on the PMS, age at which the radiative core appears, initial rotation velocity, surface rotation rate and rotation period when the radiative core appears (taken at 5% of critical rotation velocity of the corresponding model), and surface rotation velocity, surface rotation rate, rotation period, surface lithium abundance, effective temperature, and luminosity at the arrival on the ZAMS.

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