Fig. 2.
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Posterior distributions for the coefficients C⋆, Cmol and Cnorm that define the star-forming plane in each galactic environment, measured at a spatial resolution of 150 pc. As the posterior distribution of Cnorm is considerably narrower than that of C⋆ and Cmol, the x-axis has been binned in smaller bins and the distribution renormalized for an easier visualization.
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