Accretion rate vs. stellar mass for the objects with disks in the Chamaeleon I star-forming region and those in the Lupus star-forming regions studied by Alcalá et al. (2014, 2017). Symbols are the same as in Fig. 3. The upper boundary expected by theory of L_acc = L_⋆ and the lower limit imposed by chromospheric emission are shown. The blue dot-dashed box highlights the extent of the region that is empty of data, possibly as a result of photoevaporation of the disks.