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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