Fig. 9
Observed SED of HD 100546 plus photosphere (gray lines). Also displayed are a series of models with self-consistent dust settling with a turbulent mixing strength of α = 0.01, for grains with surface-to-mass ratios of σ/m = 105 cm2/g (solid line) and 4 × 103 cm2/g (dotted line), corresponding to compact grains of 0.1 and 2.5 μm, respectively.
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