Distribution of mass-loss rates and terminal velocities derived from the spectroscopic fitting by Sander et al. (2019) and Hamann et al. (2019) for an observed stellar population of galactic WR stars of nitrogen (WN), carbon (WC), and oxygen sequences (WO). Mass-loss rates and terminal velocities derived in our steady-state (log₁₀ (Ṁ∕ M_⊙ yr⁻¹) = −4.83, v_∞ = 2200 km s⁻¹) and time-dependent (log₁₀(Ṁ∕ M_⊙ yr⁻¹) = −4.78, v_∞ = 2063 km s⁻¹) simulations are consistent with the range of mass loss shown on this figure.