Grain opacity and the bulk composition of extrasolar planets - II. An analytical model for grain opacity in protoplanetary atmospheres

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Fig. 9

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MP08 comparison case. Impact of the monomer size on the opacity. Blue: 1 μm. Brown: 10 μm. Green: 100 μm. Dashed lines are from MP08, solid lines from the analytical model where the 1 and 10 μm cases lead to an identical opacity so that the lines lie on top of each other.

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