Fig. 10

Top: abundances relative to H nuclei and right-to-left
accumulated column densities of CN, HCN, and their ices in the modelled
protoplanetary disc as a function of height above the midplane at a radius of
105 AU. Also shown for species with a single 15N substitution (dotted
curves). Bottom: ratios of abundances and column densities of
14N- and 15N-bearing species. Also indicated is the
elemental ratio
(dashed line).
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