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   52123
   We propose an ASCA observation of Mrk 6 which we will use to study its
   X-ray spectrum in detail for the first time. This galaxy is classified
   as a Seyfert 1.5 and has ionization cones, an interesting radio
   morphology and a highly variable optical spectrum. As the two other
   Seyfert 1 type galaxies with ionization cones show complex absorption
   in their X-ray spectra, it appears likely that the ASCA spectrum of Mrk
   6 will reveal such absorption as well. We will quantify the amounts of
   cold and warm absorption. We will also probe the hard X-ray spectrum
   from the black hole region and will look for rapid X-ray variability, a
   broad iron line and continuum variability. The HEAO-1 flux, [O III]
   flux and far-infrared flux all suggest that Mrk 6 should be bright for
   ASCA.
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