The Influence of Bulge Profile Shapes on Claims for a Scale-free Hubble Sequence for Spiral Galaxies

We investigate recent claims that the Hubble sequence of spiral galaxies is scale-free. Fundamental to this investigation is the fact that within the photometric data of 86 spiral galaxies from de Jong & van der Kruit (1994) from which these claims were made a trend exists between morphological type and bulge profile shape. While late-type spiral bulges are described by an exponential luminosity profile, the early-type spiral bulges are better described by an r or r law. Taking the scale-lengths from the best-fitting surface brightness profile models (i.e. either using exponential, r, or r law profile parameters), we show that in all six passbands used (BVRIHK) the early-type spirals have a larger re/h ratio than late-type spiral galaxies. In contrast to this, fitting an exponential profile to the bulges of all spirals results in the mean re/h ratio for the early-type spiral galaxies actually being smaller than the mean re/h ratio for the late-type spiral galaxies (at the 3σ significance level using K-band data). Subject headings: galaxies: spiral, galaxies: structure, galaxies: fundamental parameters, galaxies: for-