  The Advanced Camera for Surveys (ACS) Fornax Cluster Survey is a Hubble Space
Telescope program to image 43 early-type galaxies in the Fornax cluster, using
the F475W and F850LP bandpasses of the ACS. We employ both 1D and 2D techniques
to characterize the properties of the stellar nuclei in these galaxies, defined
as the central "luminosity excesses" relative to a Sersic model fitted to the
underlying host. We find 72+/-13% of our sample (31 galaxies) to be nucleated,
with only three of the nuclei offset by more than 0.5" from their galaxy
photocenter, and with the majority of nuclei having colors bluer than their
hosts. The nuclei are observed to be larger, and brighter, than typical Fornax
globular clusters, and to follow different structural scaling relations. A
comparison of our results to those from the ACS Virgo Cluster Survey reveals
striking similarities in the properties of the nuclei belonging to these
different environments. We briefly review a variety of proposed formation
models and conclude that, for the low-mass galaxies in our sample, the most
important mechanism for nucleus growth is probably infall of star clusters
through dynamical friction, while for higher mass galaxies, gas accretion
triggered by mergers, accretions and tidal torques is likely to dominate, with
the relative importance of these two processes varying smoothly as a function
of galaxy mass. Some intermediate-mass galaxies in our sample show a complexity
in their inner structure that may be the signature of "hybrid nuclei" that
arose through parallel formation channels.
