Chemical and Photometric Evolution Models for Disk, Irregular, and Low Mass Galaxies
Figure 7
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.
