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   PR # 41222
   We propose to observe the cluster of galaxies A3627 which contains a
   radio galaxy as its cD galaxy. The target of this observation is to
   measure the non-thermal pressure support in the cluster. Here we
   propose to measure the non-thermal pressure with the radio lobes
   associated the cD radio galaxy. Pressure comes from magnetic field
   and high energy electron will be estimated by measuring inverse
   Compton X-ray, while thermal pressure of the hot gas filling the
   cluster will also be estimated by observing soft X-ray spectrum from
   the cluster. Thus the rest non-thermal pressure in the cluster will
   be determined with this ASCA observation.
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