Fig. 12

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Pixel-per-pixel comparison of the 12CO and H2 total column density maps. The maps are restricted to the field of observations mapped by both Spitzer/IRS, IRAM-30m, and APEX telescopes. The 12CO data points were obtained with opacity-corrected population diagrams Dell’Ova et al. (2020). The H2 data points correspond to the results obtained with the thermal admixture SE description (see Sect. 5.2). We show the best linear fit associated with the sample of data points and the corresponding H2-to-12CO molecular abundance.
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