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    PR # 32221                                                                   
     A new optical spectrum which we have obtained of the broad-line radio       
     galaxy Pictor~A reveals a prominent double-peaked component of the          
     Balmer lines which did not appear in any previous spectra. Of all the       
     X-ray bright AGNs, Pictor~A is now the one with the widest displaced        
     and symmetric twin peaks, which are separated by 14,400 km s$^{-1}$.        
     We propose to look for the Fe K$\alpha$ counterpart of this feature,        
     which could be well resolved by the SIS if it has the same profile as       
     the optical lines. Plausible interpretations of such a line include a       
     bipolar outflow or fluorescence from the surface of the accretion           
     disk. The relative strengths of the Fe K$\alpha$ and Balmer lines can       
     be used to estimate the column density of emitting material, which          
    can help to distinguish among                                                
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