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   PR #    62
   The two early type galaxies NGC4406/4374 are separated by 18'. The
   for-mer is a bright source with extended X-Ray morphology and high
   radial velocity.The other is a weak radio galaxy with jets. Two asuka
   pointings will allow usto study two morphologically similar galaxies
   under vastly different conditions.Evidence for ram-pressure stripping
   of the N4406 ISM was provided by multi-wavelength imaging studies.
   However, available kinematic data does not favorthis hypothesis. Given
   enough observed power in lines, Asuka may be able toprovide kinematic
   discrimination of the ram-pressure stripping model. Also, itprovides
   the unique capability to explore the fate of the stripped ISM: Is it
   lost to the hot ICM through evaporation, or will it cool and
   eventually condense into a tail?
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