Advances in Astronomy / 2014 / Article / Fig 3

Research Article

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

Figure 3

The ratio as a function of the mass in the disk . Our models results are the solid red dots. The cyan and black lines are the results obtained by Mateo [95] and Shankar et al. [96] from observations of the local group of galaxies and from halo data, respectively. Magenta, blue, and green dashed lines are results from Leauthaud et al. [97] for different ranges of redshift as labeled. The MWG point is represented by a blue full triangle and the dotted black line marks the limit between disk and spheroidal galaxies from González Delgado et al. [98].

You are browsing a BETA version of Click here to switch back to the original design.