A major asymmetric ice trap in a planet-forming disk - IV. Nitric oxide gas and a lack of CN tracing sublimating ices and a C/O ratio <1

Open Access

Fig. B.11

C₂H column density in the non-dust trap (north) side of the disk after 1 Myr. The models are consistent with the upper limit on the C₂H column density derived from observations except for a narrow peak at 25 AU for the models with the lowest initial H₂O abundance.

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