  X-ray images and gas temperatures taken from a deep ~200 ks Chandra
observation of the Centaurus cluster are presented. Multiple inner bubbles and
outer semicircular edges are revealed, together with wispy filaments of soft
X-ray emitting gas. The frothy central structure and eastern edge are likely
due to the central radio source blowing bubbles in the intracluster gas. The
semicircular edges to the surface brightness maps 32kpc to the east and 17.5kpc
to the west are marked by sharp temperature increases and abundance drops. The
edges could be due to sloshing motions of the central potential, or are
possibly enhanced by earlier radio activity. The high abundance of the
innermost gas (about 2.5 times Solar) limits the amount of diffusion and mixing
taking place.
