Top left: evolution of the stellar radius R_⋆ of stars from 0.3 to 1.4 M_⊙ as a function of time. Top right: surface angular velocity evolution (scaled to the present Sun angular velocity Ω_⊙ = 2.87 × 10^-6 s^-1) for the different stellar masses. Bottom left: evolution of the radius aspect ratio α = R_c/R_⋆ of stars from 0.3 to 1.4 M_⊙ as a function of time. Bottom right: evolution of the mass aspect ratio β = M_c/M_⋆ of stars from 0.3 and 1.4 M_⊙ as a function of time. Legend: the first step in each model (triangle), the ZAMS (square), and the TAMS (cross). Table 1 summarizes at which evolutionary step the models in this work stop.