Mind the trap - Non-negligible effect of volatile trapping in ice on C/O ratios in protoplanetary disks and exoplanetary atmospheres

Open Access

Fig. B.1

Same as Figure 2, but including CO trapping in CO₂. We note that for the model $F_{H_{2} O}$ $\[F_{\mathrm{H}_2 \mathrm{O}}\]$ (CO,CO₂) = 0.8, $F_{{C O}_{2}}$ $\[F_{\mathrm{CO}_2}\]$ (CO) = 0.2 there is no gas phase C/O ratios outside the CO₂ snowline because CO does not release before the CO₂ co-desorption event.

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