Similar to Fig. 5, but displaying the dependence on α_tot in the vertical axes, so each diagnostic is shown via a heat map. The fraction of dust mass accreted onto the star is also shown as an additional column on the right. Regions of the ψ_DW versus α_tot parameter space where the timescales are above given thresholds (1 Myr, 3.16 Myr and 10 Myr) are marked by dotted, dashed, and solid black lines (same scheme as Figs. 5, 6)