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Fig. 18

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Relation between the parameters describing the line richness of the RoIs and physical properties of the hosting ALMAGAL clumps. From top to bottom, the different rows show the fraction of bandwidth with line emission, the line luminosity, and the fraction of line luminosity to total luminosity. From left to right, the different columns show the size of the RoI area, the clump luminosity-to-mass ratio (Lclump/Mclump) as an indicator of evolutionary stage, and the clump dust temperature (Tdust). No significant difference is seen for the spw 0 (lighter grey) and spw 1 (darker grey) data. Black symbols in the middle and right-column panels correspond to those RoIs with area sizes larger than 3.2 × 107 au2, corresponding to the 84th percentile of the RoI area sizes shown in the left-column panels.

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