ON THE SHAPE OF THE LIGHT PROFILES OF EARLY-TYPE GALAXIES

We have obtained the best fit to the light profiles of a luminosity-li mited sample of elliptical and SO galaxies with a power law r(1/n), le tting the exponent remain free rather than keeping it fixed at 1/n = 1 /4 as in the well-known de Vaucouleurs formula. The introduction of a free parameter in the fitting formula (ranging from n = 0.5 for [r(e)] = 0.3 kpc to n = 16 for [r(e)] = 25 kpc) is justified by the existenc e of a good correlation between n and the global galaxian parameters, such as total luminosity and scale-radius. This result seems to be in line with the segregation of properties between the 'ordinary' and 'br ight' families of early-type galaxies, and has consequences for the cl aimed independence of the shape of galaxy profiles with respect to the Fundamental Plane parameters.