Fig. 13
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Grain size distribution (integrated in time) of the dust grains lost with the photoevaporative flow for the disks subject to low, medium and high FUV environments, at t = 1 Myr. The disk’s parameters are a star of 1 M⊙, initial size of rc = 90 AU, and a gap substructure at 30 AU. The location of the gap rgap is indicated with a dotted white line.
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