Fig. B.1.
Optical images of the eight H2-rich HI-undetected galaxies (Zabel et al. 2019) for which we evaluated the MH2/MHI ratio (Fig. 9). They are sorted according to increasing MHI upper limit. The g-band optical images come from the Fornax Deep Survey (Iodice et al. 2016; Venhola et al. 2018; Peletier et al. 2020). We show a 5 kpc scale bar in the bottom-right corner.
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