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   PR # 12163
      Previous observations of Mkn841 have shown one of the strongest
    signatures of Compton Reflection in a Seyfert-1 galaxy. Thus ASCA
    observations ofMkn841 are some of the most interesting and important
    which can be performed to advance our understanding of Compton Reflec
    tion in AGN. We propose a 20 ksec observation which will allow us to
    determine whether the high equivalent width Fe K line previosuly
    observed is a single line or a blend of several species, while
    comparison between the energies of spectral features observed across
    the ASCA bandpass may allow us to constrain the ionization state of
    the accretion disk.


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