  It was recently claimed that several galaxy clusters containing radial and
tangential gravitational arcs and having a measured velocity-dispersion profile
for the brightest cluster galaxy had to have central density profiles
considerably flatter than those found in CDM cluster simulations. Using a
simple analytic mass model, we confirm this result_for axially symmetric_ mass
distributions, but show that steep density profiles are well in agreement with
the cluster requiring the flattest axially symmetric profile once even small
deviations from axial symmetry are introduced.
