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   PR # 43046
   We propose an observation of the cluster A514 which shows a highly
   unusual morphology in its X-ray surface brightness distribution, has
   a very low X-ray luminosity for its optical richness, exhibits
   extensive substructure in both its gas and galaxy distributions and
   has an unusually high number of associated radio-tail galaxies. This
   cluster is a very strong candidate for an on-going merger of
   subclusters and an Asca observation provides us with an excellent
   opportunity to study in detail the very early stages of such a
   merger.
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