Fig. 14

(top) and IR8 ratio (bottom) versus
L[8 μm] for the local galaxy sample (ISO,
AKARI, Spitzer-GOALS). Galaxies with compact mid-IR (more than
60% of the light emitted at 13.2 μm within the resolution element
of 3.6″) and radio
(ΣIR ≥ 3 × 1010 L⊙) light
distributions are marked with large filled red dots. Here the solid and dashed
lines present the median and 68% dispersion around the Gaussian distribution as
defined in Eq. (4).
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