Fig. 10
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Midplane distribution of molecular abundances for CO and its tracer, N2H+, for the viscous and wind models at 1 Myr. The CO abundance dips for both at the same position as a steep increase in N2H+, which is indicative of the CO ice line. The three grey bands show the range of initial embryo radii that result in the synthetic planets b and c in the viscous and wind models.
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