Figure 5.
Violin plot representations of the resolved quantities that are studied in this paper across the Hubble types. Violin plots are histograms, where the width along the x-axis indicates the normalized fraction of data at the corresponding y-axis value. The values of ΣSFR, Σmol, |$\tau ^{\rm mol}_{\rm dep}$|, and |$\tau ^{\rm mol}_{\rm dep}$|/τorb are analysed pixel-by-pixel, while Vc and τorb azimuthal averages are calculated within 2 Reff. Choosing Vc and τorb within 1 Reff renders the trend with Hubble type of the two quantities even more prominent. White circles represent the median values for each Hubble type. Dashed lines show the global median of the full sample of galaxies for a given property. This figure shows that all quantities, except Σmol, appear to be related to the galactic morphology. These trends do not change if we include Σmol and ΣSFR from the non-detected line of sights.