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    PR # 31190                                                                   
     We propose an ASCA observation of the ultraluminous infrared galaxy I       
     RAS110548-1131 in which broad Ha (FWHM 7,600km/s) was found in the po       
     larized flux spectrum. This object is classified as a Seyfert 2. Howe       
     ver, the polarized BLR suggests the heavy nuclear obscuration and tha       
     t its radiation of the hidden nucleus would be electron-scattered int       
     o the line of sight. This object could be one of the nearest  quasar        
     which emit an intrinsic luminosity of Lx=10^45 erg/s, and then we can       
      expect the extremely large EW of the He-like Fe K line (EW =  2-3keV       
     ) on the scattered continuum of the hidden quasar nucleus,  because o       
     f its higher luminosity than nearby Seyfert 2s with much lower lumino       
     sities.                                                                     
                                                                                 
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