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   PR # 41187
   We propose ASCA observations of two powerful radio galaxies, 3C353
   and 4C+55.16, in which bright X-ray emission (>1E-11 erg/s/cm2) were
   detected with the HEAO-1 experiments. One has a large-scale radio
   structure classified as FRII, and the other is a core-dominated
   compact radio source. Despite of the large luminosities in radio and
   X-ray, optical properties of both objects do not indicate strong
   activities. Detailed X-ray spectroscopy provides information about
   central source to extend the unified model to radio-loud objects, and
   to test the relationship between X-ray nature and radio
   power/morphology.
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