Advances in Astronomy / 2014 / Article / Fig 10

Research Article

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

Figure 10

(a) The resulting spectral energy distributions—red solid lines—obtained to reproduce the observations from Hunt et al. [123]—blue open squares—for three BCD galaxies. (b) The star formation history and age-metallicity relation with which we obtain the SEDs which best fit observed spectra.