Evolutionary tracks for the stellar models (0.5 M_⊙ in blue and 1 M_⊙ in orange) considered in this work, from the end of the accreting phase to the ZAMS. The black thick lines shows the location of the ZAMS. The location on the track of the stellar models we consider in this work is highlighted by the star symbol. The other tracks of the Steindl et al. (2021) PMS grid ranging between M_★ = 0.2 M_⊙ and M_★ = 1.5 M_⊙ are shown in grey for comparison, with the structure model saved during the MESA run indicated by grey dots, yellow crosses, and teal plus signs. The crosses signal models which have a convective core while the plus signs correspond to stellar structure that are completely convective.