Fig. 3
The redshift evolution of the predicted gas-phase log(N/O) vs. log(O/H) + 12 abundance patterns within our three reference galaxies. Galaxies A, B, and C clearly show different chemical evolution of the ISM abundances with redshift. We compare our simulation with the observed average N/O–O/H relation from Dopita et al. (2016, solid grey line).
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