Fig. 8
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Evolution of the disk observables for two different stellar masses, including the gap at rc = 30 AU, with an UV flux of 103 G0. Top: evolution of the flux at the λ = 1.3 mm continuum. Bottom: evolution of the r90% radii (assuming a sensitivity threshold of 0.1 mJy beam-1). The photoevaporative radius is shown for comparison.
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