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   PR #    69
   Ginga (and BBXRT) discovered intense iron line from NGC 1068,which
   supports the Unified Seyfert model. These also provided
   valuableinformation on the structure around the AGN.On the other hand,
   Rosat HRI mapped the X-ray image and revealed the extended (about 3
   arcmin) emission.It was suggested that the extended emission from the
   starburst diskcontributed most of the hard component seen in the 2-10
   keV band.This result is contrary to the current model of electron
   scattered hard X-ray.Spatially resolved spectrum will certainly
   conclude the problem.
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