Stellar evolutionary tracks in a Rossby vs. age diagram. Shown on the figure are, 1D evolutionary track from Amard & Matt (2020) as a colour shaded envelope taking into account the initial rotational spread. The particular case of the solar track is shown in cyan colour. Symbols represent the ASH simulations and are changed according to the internal differential rotation profile achieved in the convective envelope of the simulations, either banded/quenched, solar like (fast equator slow poles) and anti-solar (slow equator fast poles). The coloured vertical bars on the left represent the magnetic states either short, decadal and no cycles.