Profile comparison for the Γ2, Γ3, and Γ4 stars. Upper panels: wind velocity profile, in solid black for the 3D averaged model of Moens et al. (2022a), red-dashed lines for the 1D PoWR^HD using the same basic parameters, dotted for the PoWR^HD changing the mass, dash-dotted for the PoWR^HD changing the luminosity value with respect to Moens et al. (2022a), lighter red for the PoWR^HD with v_Dop = 50 km s⁻¹ and boldred for the 1D PoWR approach with a β-law, from left to right for the Γ2, Γ3, and Γ4 WR stars, respectively. Middle panels: same as the upper panel but for the density profile. Lower panel: same as the upper panel but for the gas temperature.