Combined effect of stellar properties and total disk gas mass on the equilibrium solution when varying the parameters M_⋆ and L_⋆ together, all the way from accreting brown dwarfs to Herbig stars. The total disk gas mass depends on the stellar mass and is such that M_disk = 0.05 M_⋆. The “star 1” case (blue) corresponds to a star of mass M_⋆ = 0.05 M_⊙ and bolometric luminosity L_⋆ = 2 × 10⁻³ L_⊙. The “star 2” case (dark orange) corresponds to a star of mass M_⋆ = 0.1 M_⊙ and bolometric luminosity L_⋆ = 8 × 10⁻² L_⊙. The “star 3” case (green) corresponds to a star of mass M_⋆ = 0.3 M_⊙ and bolometric luminosity L_⋆ = 0.2 L_⊙. The “star 4” case (red) corresponds to the fiducial model where the stellar mass is M_⋆ = 1 M_⊙ and the bolometric luminosity is L_⋆ = 2 L_⊙. The “star 5” case (purple) corresponds to a star of mass M_⋆ = 2 M_⊙ and bolometric luminosity L_⋆ = 20 L_⊙. The panels show the various steady-state profiles of some key quantities, for the model parameters M_disk= 0.05 M_⋆, a_dust = 1 μm, f_dg = 10⁻², and α_hydro = 10⁻⁴. Panels (a)-(f) show the same key quantities as in Fig. 7.