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   51146
   The discovery of the broad and skewed iron K line profiles in many
   Seyfert 1 galaxies shows that the line is emitted in the innermost
   region of the accretion disk around the central suppermasive blackhole.
   On the other hand, up to now there is no report to detect the similar
   iron line profile in quasars. This can be due that the central region
   in quasars is different from that in Seyfert galaxies. Here we propose
   to observe the nearby quasar H 1846-786. From this observation, we will
   search the diskline profile of the iron line in the quasar and clarify
   whether the physical condition close to the central engine is similar
   or different between Seyfert galaxies and the more luminous quasars.
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