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Fig. 5.

image

Spectra energy distributions per unit SFR for galaxies in scenarios B0 (left panel) and K0 (right panel). The luminosity divided by the SFR, is plotted, where ε is the photon energy and Lε is the specific luminosity, to simplify the comparison between galaxies of different SFRs. The solid and dashed lines correspond to = 200 and 0.005 M yr−1, respectively. The colour lines represent the individual contributions from different mechanisms (the colour code is the same as in Figs. 3 and 4), whereas the black lines show the total SED. The grey shaded region indicates the Fermi energy range.

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