Advances in Astronomy / 2014 / Article / Fig 5

Research Article

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

Figure 5

Evolution with redshift of the surface density of diffuse gas, , molecular gas, , and stellar mass, , in , in top, middle-top, and middle-bottom rows, and the star formation rate, , in , in the bottom one. All in logarithmic scale. Each column shows the results for a theoretical galaxy of the Table 1, from the galaxy, with , to the most massive one for . Each line corresponds to a different redshift: purple, blue, cyan, green, magenta, orange, and red for 5, 4, 3, 2, 1, 0.4, and 0, respectively.