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   PR # 12034
    We propose to study Fe emission lines and absorption edges in three
    hard X-ray selected narrow emission-line galaxies.All 3 already have
    detected Fe K emission lines(in unpublished Ginga data), and their in
    trinsic columns are large enough so that Fe edge absorption features
    are also detectable.Indeed, our simulated spectra show that Fe K
    emission and absorption features will be detected with ASCA in all
    three sources.The high spectral resolution of the ASCA SIS and GIS
    detectors,and large effective area near 7 keV,will enable strong cons
    traints on the ionization state,the iron abundance, and the covering
    factor.Further, the 0.5--2 keV capability of ASCA coupled with the
    high intrinsic $N_H$ will set very strong constraints on any low-
   energy components.
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