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    PR # 32159                                                                   
     We have discovered several luminous X-ray galaxies whose optical            
     spectra, dominated by starburst signatures, have only weak traces of        
     Seyfert activity.  These starburst/Seyfert composite galaxies are           
     also luminous IR sources. The closest and brightest composite, $IRAS$       
     00317-2142, has a disturbed morphology indicative of a prior                
     interaction. We propose that the starburst/Seyfert composites are           
     Seyfert analogs to the Sanders et al.\ (1988) evolutionary sequence         
     tying quasars to ultraluminous IR galaxies, in the stage when the AGN       
     is just beginning to penetrate its enshrouding layer of gas and dust.       
     An $ASCA$ observation of $IRAS$ 00317-2152 will test this hypothesis,       
     undoubtedly shedding new light on the connection between starburst          
    and Seyfert activity in galaxi                                               
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