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.3

Abundance of gas (left) and ice (right) phase species in the dust trap side model of the IRS 48 disk. Top row presents the H₂O abundance, the second row that of OH, the third row that of CN, the fourth row shows C₂H, and the final row shows NH₃.

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