Fig. 5: Comparison between the different disk-mediated accretion histories for the standard input physics.

a Evolution in a Hertzsprung-Russell diagram of eight chosen models. These models have been selected to show the extent in the Hertzsprung-Russell diagram reached by different accretion histories while minimising the overlap between lines. See Supplementary Fig. 37 for a version with all models. b The distribution of frequency values in the 34 models for the pre-main sequence phase. The frequency differences are presented as violin plots grouped according to the radial order. In this type of plot, each horizontal line corresponds to the value of one model and a kernel density estimate calculated with a bandwidth of 0.3 on each side leads to a violin-like shape. Violins are plotted green if the modes are excited in most of the models or salmon if they are stable. The grey areas mark the Rayleigh limit corresponding to 4 year Kepler (dark grey) and 357 days TESS light curves (light grey). The colours of the evolutionary tracks in the top panel are chosen without specific reasoning and are only to allow discrimination between the models. c Distribution of frequency values at the ZAMS.