H I-bearing dark galaxy predictions from constrained Local Group simulations: How many and where to find them

Open Access

Fig. 1.

M_★–M_halo relation for isolated galaxies within our simulated Local Group analogues, containing gas and stars and with DM halo masses between 10⁹ M_⊙ and 10^12.5 M_⊙. Galaxies from the HESTIA simulations are coloured in shades of blue, and galaxies from NIVARIA-LG in red. The M_★ − M_halo relations from Moster et al. (2013), Brook et al. (2014), and Girelli et al. (2020) are shown in dotted-dashed, dashed, and dotted lines, respectively.

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