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Radial distribution of dust, stars, gas, and star formation rate in DustPedia face on galaxies

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Figure

Table 1. Main properties of the galaxy sample.
Table 2. Main properties of the Herschel images and the ancillary ones used for this work.
Table 3. Collected Hi 21 cm and 12CO (1–0 or 2–1) emission line data used to derive the mass surface density of the atomic and molecular gas,respectively.
Fig. 1. Example SED fits: the datapoints are from three disitions on NGC 5457 (M 101) atfferent po- R ≈ 0.3, 0.5, and 0.7 × r25, corre-sponding to the local average heating conditions (fitted U ≈ 3, 2 and 1,respectively, from top to bottom).
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