Fig. 1.
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Distributions of mass of the full sample of galaxies and the galaxies hosting a significant CRD. Panel (a): Distribution of stellar mass confined within the disk region, independent of the circularity parameter. Panel (b): Distribution of the total mass according to the Subfind algorithm (i.e., considering all particles bound to the galaxy). In both panels, the distribution was normalized according to the full sample of 260 galaxies, represented by the light blue shaded distribution. The orange shaded region represents the distribution of the 26 galaxies hosting a significant CRD component.
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