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   71110
   One of the best way to probe the central region of AGNs will be to
   observe iron line features in X-ray spectra. Seyfert 1 galaxies
   generally show a broad and skewed feature around 5-6 keV and it is
   interpreted as fluorescent lines from the innermost region of accretion
   disks. We propose to measure iron line features in radio galaxies and
   to compare them with those of Seyfert galaxies to investigate
   differences of the central part of jet ejecting AGNs from that of non-
   jet AGNs. As a part of this study, we propose a supplementary
   observation of 3C382, from which some evidence of iron line has already
   been obtained but no detailed information was extracted due to poor
   statistics.
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