The visual surface brightness of K/M giants and dwarfs with near-solar meta
llicity differ slightly in agreement with the gravity effects predicted by
recent theoretical models. We show that M-dwarfs display also a metallicity
dependence of the surface brightness in the infrared ii-band in agree ment
with theory. Based on these results, we present improved Barnes-Evans type
relations and estimate the radii of 60 single or presumed M and K-dwarfs.