Fig. 22.
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Star formation rate surface density (ΣSFR) as a function of dense gas fraction (Fdense) in NGC 1068 measured at 100 pc scales compared to the data obtained in other galaxies (symbols as in Fig. 8). Vertical and horizontal error bars at the lower-right corner account for the typical uncertainties, which amount to ±0.09 dex and ±0.13 dex, respectively.
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