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Fig. 10


Specific radial torque density in units of (dΓ/dm)0 for 2D and 3D embedded planet models using different mass ratio and disk temperature. The first two curves are identical to those in the previous figure, and the third is a fit presented by D’Angelo & Lubow (2010) corresponding to the model with T(r) ∝ r-1 and Σ(r) ∝ r−1/2.

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