Fig. 6.
Mean r-band surface brightness within three effective radii, ⟨μr⟩, as a function of the stellar mass for the local sample of Hα emitters. The color scale shows the apparent magnitude of the sources. The hatched area marks a surface brightness larger than 24 mag arcsec−2. The vertical dotted line marks a stellar mass of log M⋆ = 9.
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