The results for the wind from the differentially rotating central star with the fixed stellar parameters given in the upper part of the table. The converged values of the wind parameters v_∞, β, , γ, δ, , and mass-loss rates log   Ṁ, together with the critical radius , which is equal (i.e. close) to the sonic radius (obtained by ISA-Wind), are displayed in the lower part of the table: the results of the first column (at the pole) correspond to the spherical 1D wind model published in Paper I (see Table 5), whereas the second and third column represent the converged parameters of the iteration cycles shown in Table A.1 at the equator for the different stellar rotation speeds of V_rot = 300 and 500 km s^-1, respectively. In addition, the terminal ratios (ρ_eq/ρ_p)_∞ of the wind densities at the equator compared to the pole are also calculated.