Fig. 6.From: Star formation and dust extinction properties of local galaxies as seen from AKARI and GALEXContributions of FUV and SF-related dust luminosities to SF luminosity. The left panel shows the contribution of FUV luminosity to the SF luminosity, and the right panel shows the contribution of the dust luminosity. Downward and left-pointing arrows represent galaxies which have UV flux densities below the detection limit of GALEX.Back to article page