From top to bottom: extended profiles for the density (blue dots), temperature (blue squares for temperature inversion by Harper et al. (2001) also known as ‘Harper’, and red circles for simple radiative equilibrium), wind velocity (purple), and Rosseland optical depth (green). The extended model with log L/L_⊙ = 4.8, T_eff = 3500 K, log g = 0.0, M = 15 M_⊙, M_⊙ yr⁻¹, and R_max = 8.5 R_* corresponds to the stellar parameters of HD 95687.