Modified wind-momentum rate computed using GA best fit values compared to the predictions made by Leuven (Björklund et al. 2021), Krtička (Krtička & Kubát 2018), and Vink (Vink et al. 2001) for each star in our sample. Supergiants are blue squares, giants are orange triangles, and dwarfs are green circles. A linear fit to the wind momentum calculated using the GA best-fit values for stars with log(L/L_⊙) ≥ 5.0 is shown by the solid line. Theoretical predictions tailored to our best-fit stellar parameters from Vink (Vink et al. 2001) and Leuven (Björklund et al. 2021) are shown in dotted and dashed lines, respectively. Theoretical predictions for LMC stars from Krtička (Krtička & Kubát 2018) are shown with the dash-dotted line, although these are not tailored to the GA results.