Fig. 11
Atmospheric chemical compositions of a HD 209458b with a C/O ratios 3× (top) and 6× (bottom) solar obtained with the full scheme of Venot et al. (2012; solid lines) and the reduced scheme (dotted lines). Deviations are easily visible at pressures lower than 10 mbar. The abundance of C2H2 has been determined with the full scheme only, as this species is not included in the reduced scheme.
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