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    PR # 31180                                                                   
     ASCA results obtained for the Sey2 NGC5252 (Cappi et al. 1994) show a       
      very flat spectrum (1.5), i.e. apparently a dominant reflection comp       
     onent, with little evidence for an iron emission line. It contradicts       
      the last ASCA results for the Sey2 NGC1068, Mkn3 and NGC6552 which c       
     onfirm the presence of a flat hard X-ray continuum together with a ve       
     ry strong fluorescent iron line which are commonly interpreted as the       
      signature of a reflected emission from cold matter. Our results pres       
     ent a problem for simple unified models. It could be explained if one       
      assumes that Sey2 are intrinsically different than Sey1 as indicated       
      by recent combined GINGA/OSSE data (Zdziarsky et al. 1994). To furth       
     er investigate on this excyting controversy, we propose 2 ASCA observ       
    ations of the Sey2 NGC7674 and                                               
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