Fig. 5.
Histograms showing the distribution of the deconvolved diameters of the dusty molecular tori (or polar components) derived from the combined sample of NUGA and GATOS (gray-filled histograms). We adopt for GATOS the average sizes estimated from the MSR and HSR datasets. The blue-filled histogram identifies the distribution of sizes of the tori derived for NUGA galaxies (Combes et al. 2019).
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