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    PR # 31541                                                                   
     We propose to use ASCA to detect, allow examination of, the buried qu       
     asar nucleus in the narrow line radiogalaxy PKS 0634-205.  Our observ       
     ations will allow us to determine the intrinsic quasar lunin- osity a       
     nd the foreground column density, and compare them with predictions f       
     rom optical-near-infrared data.  This mulit-wavelength analysis will        
     allow us to examine PKS 0634-205's place in the  Standard Model for r       
     adiogalaxy-quasar unification, and will also have far more general im       
     plications for the unification of broad and narrow line objects.            
                                                                                 
                                                                                 
                                                                                 
                                                                                 
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