  We investigate the relation between the X-ray nuclear emission, optical
emission line, radio luminosity and black hole mass for a sample of nearby
Seyfert galaxies. Strong linear correlations between the 2-10 keV and [OIII],
radio luminosities have been found, showing the same slopes found in quasars
and luminous Seyfert galaxies, thus implying independence from the level of
nuclear activity displayed by the sources. Moreover, despite the wide range of
Eddington ratios (L/L(Edd)) tested here (six orders of magnitude, from 0.1 down
to 10^(-7), no correlation is found between the X-ray, optical emission lines,
radio luminosities and the black hole mass. These results suggest that low
luminosity Seyfert galaxies are a scaled down version of luminous AGN and
probably are powered by the same physical processes.
