Notes. With respect to the stellar and wind parameters determined by Crowther et al. (2010) (cf. Table 12), the main difference to the parameters of our prototype model – model “A⁺” – is the mass of the object M_∗. From our analysis it turned out that the mass must be lowered by almost 30% in order to reproduce the dynamical parameters and the UV spectrum of the star. By means of the parameters determined by model “A” we show further, that the problem of a too high terminal velocity v_∞ (cf. Table 12) can not been solved just by a moderate reduction of M_∗ and an additional enhancement of the abundances of the elements which increase Ṁ (cf. Pauldrach 1987) – namely iron and nickel –, because although Ṁ increases in this case to the required value, v_∞ remains at a value which is still too high.