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Fig. 21.

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Relation between the star formation rate surface density and the molecular gas surface density at scales of ≃100 pc. Different symbols indicate different galaxies. The solid black line shows the best fit obtained by Bigiel et al. (2008) (scaled to the same XCO conversion factor) for the Heracles sample of nearby galaxies using star formation rates derived from Hα+24μm flux surface densities. The dotted lines show lines of constant star formation efficiency, indicating the level of ΣSFR needed to consume 1%, 10%, and 100% of the gas reservoir (including helium) in 108 years, corresponding to depletion times of 108, 109, and 1010 years.

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