Fig. 18
Integrated dust and PAH emission SEDs for the diffuse component, for model galaxies
with different contribution from the old stellar population (plotted as different
curves in each panel). All models shown in this figure are for pure
disk galaxies (B/D = 0.0). From left to
right the panels show model galaxies with various levels of
SFR (SFR′ = 0.0, SFR′ = 2.0 and
SFR′ = 20.0). From top to bottom the panels show
models with various face-on B band opacities
(
,
, and
). The colour coding is as
follows: green is for old = 0.0, red is for
old = 2.0, blue is for old = 10.0 and black is for
old = 20.0.
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