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    PR # 31141                                                                   
     We propose the radio lobes of the galaxy Centaurus B to observe with        
     ASCA to determine the magnetic fields therein. During the previous  p       
     hase of the ASCA guest observations, we observed another radio galaxy       
       Fornax A (PI=Makishima) and discovered the X-ray emission from the        
      radio lobes. The obtained spectrum strongly suggests that the X-ray        
      emitted via inverse-Compton scattering. These results with reported        
      radio flux allowed us to determined the magnetic field in the lobes        
      without any assumptions. Here we propose to observe brighter radio         
     galaxy Centaurus B to determine the magnetic field. The jets and  lob       
     es spread upto 12 arcmin and brighter radio emission suggest us  to b       
     e able to have detailed study of the magnetic field structure  of jet       
    s and lobes in AGNs.                                                         
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