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Fig. B.2


Left panel: best-fit model midplane temperature obtained from fitting each wavelength separately (solid lines, one line per each wavelength) or from our multiwavelength fit (dashed line). Right panel: for the same best-fit models, the optical depth τν = κνΣ of the disk midplane to its own thermal radiation. Both panels: the single-wavelength fits have been performed assuming a constant amax = 1.3 mm (i.e., constant dust opacity) throughout the disk. The dashed lines refer to the best-fit model obtained through multiwavelength modeling.

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