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   PR # 41092
   We propose to observe the radio lobes of the galaxy NGC 612 to detect
   the inverse-Compton (IC) X-rays from the lobe. By estimating the flux
   of IC X-rays and comparing with the radio flux of synchrotron
   radiation, we can determine the magnetic field strength in the lobe
   without any assumptions. Because we can also estimate the electron
   energy density in the lobe from the flux of the IC component itself,
   it will be confirmed whether the energy equipartition between
   particles and fields will hold in the lobe or not. Through this
   observation, we will also discuss on the pressure balance between the
   lobes and the galactic haloes.
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