Chemical and Photometric Evolution Models for Disk, Irregular, and Low Mass Galaxies
(a) Radial distributions of the surface density of diffuse gas, , molecular gas, , and stellar mass, , in , and the star formation rate surface density, , in , all in logarithmic scale, for the least massive galaxy of our example table, with . (b) Evolution with redshift of radial distributions of elemental abundances, C, N, O, and Fe of the same galaxy.
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