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Fig. 5

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Histogram for stellar accretion rate vs. disc mass at 2Myr and the same synthetic disc populations shown in Fig. 4. The observed data from the Lupus (in red) and Chamaeleon I (orange) star forming regions from Manara et al. (2019) are shown for comparison. Two disc dispersal timescales τ = G/MG of 1 Myr and 10 Myr (assuming that the gas disc mass MG is 100 times the observed dust mass) and the best fit to the data from Manara et al. (2016b) are shown as well.

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