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   PR # 12096
    The X-ray spectra of Seyfert galaxies have absorption and emission
    features which are attributed to reprocessing by cool material,hypoth
    esized to be the accretion disk.If this view is correct,the Fe~K$\alp
    ha$ fluorescence line should be broad and possibly double peaked, re-
    vealing the kinematic signature of the rotating disk.However,the best
    candidates for displaying disk-like Fe~K$\alpha$ lines may {\it not}
    be the Seyfert galaxies, but rather the broad-line radio galaxies
    (BLRGs).The BLRGs have {\it optical} emission lines that are twice as
    wide as those of their radio-quiet counterparts,and our line-profile
    studies show that disk-like Balmer lines are found almost exclusively
    in BLRGs.We propose to observe three BLRGs in order to characterize
   their spectral features.
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