Fig. 7

Top: abundances relative to H nuclei and left-to-right accumulated column densities of the isotopologues of N and N2 in the modelled interstellar cloud. Bottom: ratios of abundances and column densities of 14N- and 15N-bearing species. Also indicated are the adopted elemental ratios of 14N / 15N and 14N2 / 14N 15N (dashed lines).
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