Fig. 4
Predicted fluxes at 1 mm (F1 mm) and the spectral index between 1 and 3 mm (α1 − 3 mm) after 1 Myr of dust evolution, without radial drift, vf = 10 m s-1 and for all other parameters discussed in Sect. 2.3. Black dots with error bars are millimeter observations of the young BD ρ-Oph 102 (Ricci et al. 2012) and 2M0444+2512 (Ricci et al. 2013).
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