Fig. 10
ΣSFR and ΣMH2 of 3C 236 (triangles), the Nesvadba et al. (2010) sample (diamonds), and young sources 4C 12.50 and 4C 31.04 (squares). The bottom panel is a zoom on the area marked with a dotted box, into which most of the SFR estimates of 3C 236 fall. Solid line: best-fit of the KS law from Kennicutt (1998). Dashed lines: dispersion around the KS law best fit for normal star-forming galaxies (Roussel et al. 2007; Kennicutt 1998).
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