Chemistry across dust and gas gaps in protoplanetary disks - Modelling the co-spatial molecular rings in the HD 100546 disk

Open Access

Fig. B.7

C₂H (top row) and NO (bottom row) abundance for different C/O ratios. From left to right: C/O = 0.4 (fiducial value), 0.99, and 1.01. Only the regions with a gas number density above 10⁵ cm⁻³ are shown. The white contour indicates the NO snowline.

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