Chemical and Photometric Evolution Models for Disk, Irregular, and Low Mass Galaxies
Evolution with redshift of radial distributions of elemental abundances, C, N, O, and Fe from top to bottom. Each column shows the results for a theoretical galaxy of Table 1, from the galaxy, with , at left to the most massive one with at the right. In each panel distributions for 7 redshifts are shown, with the same color coding as in Figure 5.
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