Advances in Astronomy / 2014 / Article / Fig 6

Research Article

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

Figure 6

The evolution of the half mass radii, , as a function of the redshift for models with efficiencies sets from to 9 and for mass distribution numbers from 10 to 44 (see Tables 1 and 2 from MD) corresponding to maximum rotation velocities in the range [80–400] . Black, gray, green, red, orange, magenta, purple, cyan, and blue dots correspond to 1, 2, 3, 4, 5, 6, 7, 8, and 9, respectively.
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