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    PR # 32201                                                                   
     That there are hardly any ``narrow-line QSOs'' is important to     co       
     nsider with regard to unified models of AGNs. It is interesting to as       
     k whether the few certifiable narrow-line QSOs are intrinsically   la       
     cking in broad-line clouds, or whether they contain obscured broad li       
     ne regions similar to the hidden Seyfert 1 nuclei which are so     sp       
     ectacularly revealed in hard X-ray spectra.  We have found an      ex       
     cellent example of a narrow-line QSO among the objects in the      RO       
     SAT/IRAS All-Sky Survey.  If Asca finds a strong Fe line or an     ab       
     sorbed hard X-ray continuum, it will indicate an obscured nucleus  th       
     at is the most luminous one seen to date.  If not, then it means   th       
     at we are seeing an intrinsic narrow-line QSO, a challenge to      un       
    ified models. Comparison with                                                
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