Fig. 10.
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Mbar/M200 ratio normalized to the cosmological baryon fraction (fbar, cosmic). LSB-D is compared against a set of nearby disk galaxies (Mancera Piña et al. 2022a) and the semi-empirical relation from Calette et al. (2021), which uses abundance matching to link M⋆ with M200 and empirical correlations for Mstar/Mgas. Galaxies are colour coded according to their gas-to-baryon content (Mgas/Mbar).
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