Fig. 11
(Left) Radial profiles of optical thickness for two runs: reference and iceless. For comparison, the light shaded region shows the profile of a model of the Vega disk (Müller et al. 2010), radially scaled so that the outer edges match. The dark shaded region marks the extent of the belt of parent bodies. (Right) Size distribution of the reference run at distances of 50, 100, 150, and 200 AU.
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