Fig. 8
Comparison of the predicted fluxes at 1 mm (F1 mm) and the spectral index between 1 and 3 mm (α1 − 3 mm) for two different disk masses (Mdisk = 2 MJup-star points and Mdisk = 5 MJup-dot points). Time-evolving data from right to left (from 0.1–5.0 Myr as Fig. 7). Case of Rout = 15 AU, p = 0.5, αturb = 10-3, vf = 10 m s-1, and A = 0.4.
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