Fig. 3
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Evolution in the Rgas(90%)/Rdust(90%) vs. Rdust(90%) space for some test substructured disks evolved with DustPy code in a low viscosity regime (α = 10−3.5) for different values of the characteristic radius rc. The points associated with each trajectory represent the snapshots taken at 0 Myr, 1 Myr, 2 Myr, and 3 Myr, respectively. Solid line: External photoevaporation (FFUV = 4 G0). Dashed line: No external photoevaporation (FFUV = 0 G0).
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