Hertzsprung-Russell diagrams showing different evolutionary tracks for solar metallicity together with different predictions for the location of the TAMS as indicated in each legend. The top panel includes tracks with no initial rotation, and in the bottom panel the tracks correspond to v_ini/v_crit ≈ 0.4. Intervals of the same age difference are marked with different symbols. The gray density mesh in the background is based on a Gaussian kernel and includes our sample stars up to 2500 pc. Evolutionary tracks are limited up to the RSg phase (if applicable).