Fig. 11
The radio-infrared correlation diagram for LG dwarfs and comparison dwarfs (plotted with the same symbols as in Fig. 7), and for the sake of reference, the sample of galaxies observed by de Jong (1967) plotted as stars. The surface brightness at 2.64 GHz and at 60 μm is used (in Jy/◻′). The solid line is an orthogonal fit to the reference galaxies.
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