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   61150
   We detected an ionized iron line from NGC4579 in spite of very low
   luminosity Lx=1.4E41ergs/s by a 30ksec ASCA observation. The center
   energy of the line (6.7keV) is significantly higher than 6.4keV which
   is typical for usual Seyfert 1 galaxies. We propose detailed
   measurements of iron line profiles in the low luminosity Seyfert 1
   galaxy NGC4579. We investigate dynamical and ionization structure of an
   accretion disk in this remarkable Seyfert galaxy using line profiles
   and center energy. We also determine size and density of a disk
   comparing our X-ray results with blackhole mass determined with HST
   STIS data.
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