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

Figure 9

(a) The star formation Ψ(𝑡) and iron enrichment [Fe/H](𝑡) evolution with redshift 𝑧 for the radial regions located at 𝑅_𝑐 of models of Table 1. (b) The resulting spectral energy distributions, 𝐹_𝜆(𝜆,𝑡=13.2Gyr) obtained for the same radial region and galaxy model compared with the fiducial templates from Coleman et al. [106].

(a)

(b)