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   61160
   ASCA observations have revealed the nature of hard X-ray emission from
   Seyfert 2 galaxies which is well explained by the Unified Seyfert
   model. Soft X-ray emission is clearly seen as well as the hard X-ray
   emission. The photon indices of the soft components are widely
   distributed, and their luminosities do not well correlate with the hard
   band luminosities. This indicates that the origin of the soft X-ray
   emission is not simple. Our objective is to reveal the nature of the
   soft X-ray emission using the ASCA. We selected two nearby Seyfert 2
   galaxies (cz<1500km/s). Together with spatial information obtained from
   the ROSAT HRI observations, this should make clear the nature of the
   scattering region and the evolution of AGN.
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