Fig. 8
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Slope of the MD−Ṁ* correlation with ϕ = 0.8, ω = 0.8, and t = 3 Myr. The colored dots are Monte Carlo simulations of 105 protoplanetary disks ruled from Eqs. (4) and (5), where M0 follows Eq. (9) and tacc,0 follows a lognormal distribution centered on the natural logarithm of 2 Myr with a spread of 0.13 dex. The black line represents Eq. (D.6).
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