  We investigate the fractal structure of $2d$ quantum gravity coupled to
matter by measuring the distributions of so-called baby universes. We
demonstrate that the method works well as long as $c \leq 1$. For $c >1$ it is
not clear what distribution to expect. However, we observe strikingly similar
distributions for various kinds of matter fields with the same $c$. This
indicate that there might be some range of $c >1$ where the central charge of
the matter fields alone determines the fractal structure of gravity coupled to
matter. The hypothesis that the string susceptibility $\g = 1/3$ is found to be
compatible with the data for $1 < c \leq 4$.
