Fig. 9
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Azimuthally averaged radial profiles of simulations with different accretion rates fA > 0.5 at Mp = 2.3 MJ. (a) Total gas density (solid), CH4 vapor density (dashed) at the indicated planet mass over the unperturbed density gas and pebble profile Eq. (12). (b) C/O ratio in the gas (midplane) in our simulations based on the abundance assumed in Table 1. (c) Expected C2H column density.
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