Evolutionary tracks followed across the Hertzsprung-Russell diagram for model stars without rotation, assuming the mass-loss rates given originally from Vink et al. (2000, dashed lines, i.e., classical tracks) and those Ṁ_sc given by the self-consistent wind solutions from Gormaz-Matamala et al. (2022, continue lines, i.e., self-consistent tracks). Black dots represent: (i) the ZAMS-point, (ii) where Ṁ_sc switches to Ṁ_Vink, and (iii) the end of the H-burning stage.