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Table 4

Mean mass fluxes during the critical-rotation phase for stars with Ωinicrit = 0.95.

Z M Fluxpol Fluxeq Fluxmech Fluxeq/Fluxpol Fluxmech/Fluxpol
M M yr-1 sr-1 M yr-1 sr-1 M yr-1 sr-1

0.002 7 1.854 × 10-11 2.790 × 10-12 4.711 × 10-10 0.15 25.4
0.002 9 2.242 × 10-10 3.372 × 10-11 2.658 × 10-9 0.15 11.9
0.002 12 1.609 × 10-9 2.420 × 10-10 1.148 × 10-8 0.15 7.13
0.002 15 4.657 × 10-9 7.005 × 10-10 3.533 × 10-10 0.15 0.23
0.006 7 1.296 × 10-11 1.950 × 10-12 7.878 × 10-10 0.15 60.8
0.006 9 2.030 × 10-10 3.053 × 10-11 9.247 × 10-10 0.15 4.02
0.006 12 2.323 × 10-9 3.496 × 10-10 3.899 × 10-9 0.15 1.68
0.014 7 1.003 × 10-11 1.509 × 10-12 2.148 × 10-10 0.15 21.4
0.014 9 1.680 × 10-10 2.528 × 10-11 6.685 × 10-10 0.15 3.98

Notes.Mean polar and equatorial mass fluxes due to radiative winds (Cols. 3 and 4 respectively), mechanical mass flux (Col. 5), polar to equatorial mass-flux ratio due to anisotropic winds (Col. 6), and polar to mechanical mass-flux ratio (Col. 7). We only consider here models for which we included a radiative mass-loss prescription during the MS (Mini ≥ 7 M).

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