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   PR # 12241
    We propose to observe Fe K line profiles in three X-ray selected Sey-
    fert 2 galaxies (or NELG's; of which there are none in the PV phase)
    in order to determine whether the lines are narrow (FWHM a few x 10^3
    km/s),broad(FWHM a few x 10^4 km/s),or a combination of both.Already,
    the Seyfert 1 galaxy NGC 4151 has shown a strong narrow Fe K line and
    possible broad component.These Seyferts are 3 of the 10 brightest AGN
    in Fe K line emission and thus give the best opportunity to resolve
    line profiles. ASCA will also provide medium resolution data of the
    soft X-ray excess components known to exist in these objects.If the
    excesses are dominated by Fe L line emission then both Fe L & K energ
    ies and flux ratios will measure the state and distribution of the
   matter near Seyfert nuclei.
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