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. 12

NO abundance after 100 yr in the dust trap model with an initial NO abundance of 10⁻⁵. Most of the NO is hidden below the τ_{dust, 0.85 mm} = 1 surface at 0.85 mm indicated by the red contour. The blue contour indicates τ_{dust, 100 μm} = 1 at 100 μm, representative of the wavelength of the H₂O and OH upper limits.

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