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Fig. 2

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Boundaries of the evaporating layer: (Rmin plus signs connected in purple and Rmax, crosses connected in green) for Case A (fiducial case). We present the 16 stars of the hybrid model at 2 Myr by Baraffe et al. (2017). The dust is not evaporating where R > Rmax and the dust-free region is located at R < Rmin. Also we present an estimate of the lower threshold of inc where we expect models producing dips for each of the stars in the sample.

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