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   PR # 22152
    We have targeted the Seyfert I galaxy NGC 7314 for study with ASCA in
    order to search for evidence of the elusive accretion disk which is a
    pillar of contemporary models of AGN. Such eveidence has, to date,   
    been sparse.  In particular, the accretion disk hypothesis predicts  
    that the energy of the Fe K line in AGN should have a range of values
    less than 6.4 keV due to gravitatioanl and Doppler shifts yet nearly 
    all observations indicate energies of 6.4 keV or higher. NGC 7314 is 
    a possible exception and its X-ray spectrum is known to exhibit      
    dramatic rapid variability.  We propose to measure the energy and    
    width of the Fe K line and search for short term variability. We will
    also obtain the first spectral measurements of the continuum below 2 
   keV which may arise from repro
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