Fig. 14.
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Emission line luminosity (L′line) ratios of CO J:1–0, CO J:7–6, and [C I] 2–1 as a function of radius in galaxies W (red) and T (blue), measured in kpc-scale apertures matched to the beam size. In each panel the solid lines in the corresponding colour show the prediction if the galaxy integrated line flux ratio was valid over all individual apertures.
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