Deep spectroscopy in nearby galaxy clusters: III Orbital structure of
  galaxies in Abell 85
  Galaxies in clusters are strongly affected by their environment. They evolve
according to several physical mechanisms that are active in clusters. Their
efficiency can strongly depend on the orbital configuration of the galaxies.
Our aim is to analyse the orbits of the galaxies in the cluster Abell 85, based
on the study of the galaxy velocity anisotropy parameter. We have solved the
Jeans equation under the assumption that the galaxies in A85 are collisionless
objects, within the spherically symmetric gravitational potential of the
virialized cluster. The mass of the cluster was estimated with X-ray and
caustic analyses. We find that the anisotropy profile of the full galaxy
population in A85 is an increasing monotonic function of the distance from the
cluster centre: on average, galaxies in the central region (r/r200 < 0.3) are
on isotropic orbits, while galaxies in the outer regions are on radial orbits.
We also find that the orbital properties of the galaxies strongly depend on
their stellar colour. In particular, blue galaxies are on less radial orbits
than red galaxies. The different families of cluster galaxies considered here
have the pseudo phase-space density profiles Q(r) and Qr(r) consistent with the
profiles expected in virialized dark matter halos in $N$-body simulations. This
result suggests that the galaxies in A85 have reached dynamical equilibrium
within the cluster potential. Our results indicate that the origin of the blue
and red colour of the different galaxy populations is the different orbital
shape rather than the accretion time.
