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Table 2.

Overview of our two-dimensional simulations of main-sequence stars of different masses.

Name fov tmax tmax/τconv MCZ, i Mmixed, i Mixing rate Rib
H2.0 0 6 ⋅ 107 90 0.27 0.27 2.0 ⋅ 10−5 662
H2.0-ov0.5 0.005 5 ⋅ 107 80 0.29 0.32 1.2 ⋅ 10−5 1970
H2.0-ov1.0 0.01 7 ⋅ 107 80 0.30 0.37 2.9 ⋅ 10−8 5936

H1.5 0 1.8 ⋅ 108 180 0.09 0.09 3.0 ⋅ 10−6 1325
H1.5-ov0.25 0.0025 1 ⋅ 108 130 0.10 0.12 1.9 ⋅ 10−6 7407
H1.5-ov0.5 0.005 1.4 ⋅ 108 130 0.12 0.14 3.0 ⋅ 10−7 6421
H1.5-ov1.0 0.01 1 ⋅ 108 110 0.14 0.19 1.4 ⋅ 10−8 38470
H1.5-ov2.0 0.02 1.8 ⋅ 108 143 0.16 0.27 1.7 ⋅ 10−8 55122

H1.3 0 1.3 ⋅ 108 30 0.02 0.02 3.8 ⋅ 10−7 1015
H1.3-ov0.25 0.0025 1.1 ⋅ 108 130 0.04 0.05 3.9 ⋅ 10−7 2141
H1.3-ov0.5 0.005 1.5 ⋅ 108 150 0.06 0.08 6.0 ⋅ 10−8 3775

Notes. The first column gives the name of the model and follows the naming scheme of Table 1, the number behind the ‘-ov’ name appendix indicating the value of fov used in the one-dimensional model, which is given in the second column times 100. Columns 3 and 4 show the physical time at the end of the simulation in seconds and the number of convective turnovers, respectively. Columns 5 and 6 give the initial mass of the CZ and of the homogeneously mixed region in units of M, respectively. The mixing rates averaged for t >  107 s in units of M yr−1 are shown in the second but last column, while the bulk Richardson number is given in the last column.

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