  We present three new clusters discovered in the halo of M31 which, although
having globular-like colours and luminosities,have an unusually large
half-light radii, ~30 pc. They lie at projected galactocentric distances of
approx. 15 to 35 kpc. These objects begin to fill the gap in parameter space
between globular clusters and dwarf spheroidals, and are unlike any clusters
found in the Milky Way, or elsewhere to date. Basic photometric and derived
King profile fit parameters are given, and we discuss possible origins and
their relationships to other populations.
