Fig. 8
For our dwarf candidates, μ0−M relation in the V band (red squares), all known dwarfs of the Centaurus group in the survey area (gray filled squares), Local Group dwarf galaxies (dots; McConnachie 2012) and the candidates from MJB15 (black squares). The newly discovered Centaurus dwarf candidates have similar properties to those of known Centaurus dwarfs and Local Group dwarfs.
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