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Fig. 2.

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Radial profiles of the AGN disk employed in this work. From top to bottom: midplane gas density ρ, sound speed cs, disk aspect ratio h/R, and magnitude of the migration torque Γ. The migration torque assumes a secondary BH mass of mBH = 20 M. The outer migration trap lies within the star formation region, which begins at R ≃ 767 au.

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