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   PR #   133
   Centaurus Cluster is a nearby bright cluster with cD galaxy NGC4696.
   Itstemperature is 4keV, so there will be some soft X-ray lines.
   X-rayemission is found to be extended by GINGA observation. In
   thisobservation, we will get surface brightness of X-ray
   emission,temperature gradient and iron abundance distribution. In
   order toinvestigate the angular extent of the X-ray emission, we will
   spend partof the time for the offset pointings from the center of the
   Centauruscluster. In addition we also point on NGC4709, which is
   associated withCentaurus subcluster, and will get information about
   the clusterevolution.
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