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Fig. 6
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Pebble growth tracks (a), their resulting pebble opacity (b), and produced dust opacity (c) for a standard set of model runs at 5 AU (see Table 1). This figure is the same as Fig. 4 but now the mass is fixed at the default 5 M⊕ and the pebble accretion rates are varied logarithmically from 10−7−10−4 M⊕ yr−1.
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