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   PR #    46
   Three observations mapping the inner regions of the Perseus
   Cluster.The first observation will perform imaging spectroscopyon the
   cooling flow and NGC 1275. The second and third observations will map
   the cluster E and W of the core and will settle the question of
   whether there is an iron abundance gradient in the Perseus Cluster.
   They will also compare the emission from the cooler region discovered
   by ROSAT with the emission from the "normal" region the other side of
   the core.
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