Fig. 18.

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Results of our multi-Gaussian fitting for the TNG50 (orange), FIRE-2 (dark red), and MeerKAT (blue) galaxies. Top panels: Fraction of spectra modelled with N components (1 ≤ N ≤ 5). Bottom panels: Median value of the distribution of the Gaussian standard deviations computed for all line profiles modelled with N components, as a function of N. The different panels show our results for spaxels in different ranges of (inclination-corrected) H I column density, indicated at the top of each panel. The dashed and dotted curves in the leftmost panels show, respectively, the regular and irregular populations of simulated galaxies.
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