On the formation mechanisms of compact elliptical galaxies
  In order to investigate the formation mechanisms of the rare compact
elliptical galaxies (cE) we have compiled a sample of 25 cEs with good SDSS
spectra, covering a range of stellar masses, sizes and environments. They have
been visually classified according to the interaction with their host,
representing different evolutionary stages. We have included clearly disrupted
galaxies, galaxies that despite not showing signs of interaction are located
close to a massive neighbor (thus are good candidates for a stripping process),
and cEs with no host nearby. For the latter, tidal stripping is less likely to
have happened and instead they could simply represent the very low-mass, faint
end of the ellipticals. We study a set of properties (structural parameters,
stellar populations, star formation histories and mass ratios) that can be used
to discriminate between an intrinsic or stripped origin. We find that one
diagnostic tool alone is inconclusive for the majority of objects. However, if
we combine all the tools a clear picture emerges. The most plausible origin, as
well as the evolutionary stage and progenitor type, can be then determined. Our
results favor the stripping mechanism for those galaxies in groups and clusters
that have a plausible host nearby, but favors an intrinsic origin for those
rare cEs without a plausible host and that are located in looser environments.
