Equilibrium state values of R_t/R_co over stellar accretion rates. We compare the no-wind with the wind scenario for two stellar ages, τ_age = 2 Myr and τ_age = 5 Myr. The observed range of stellar accretion rates is shown for stellar ages between 1 Myr and 8 Myr. The stellar mass is 0.7 M_⊙, and B_⋆ = 0.5 kG. The horizontal dashed lines enclose State 2 (Eq. (2)). In the region of Ṁ_⋆ ∼ 10⁻⁷ M_⊙ yr⁻¹, the condition R_t ≥ R_⋆ would be violated, so these values have been excluded.