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   PR # 41181
   NGC5793 is a edge-on spiral galaxy which is seen in absorption
   against a radio continuum source ,located near its nucleus. Also,
   known as one of the inflared luminous galaxies ,but no AGN components
   have ever been detected in any wave lengths. According to the
   observation at frequencies of radio and IRAS bands , the flux at
   radio 21cm continuum is too strong compared with that of IRAS wave
   bands. It indicates that the strong non-thermal emission mechanism in
   it and that its nucleus is hidden in the dusty molecular gas which is
   often seen in the Seyfert 2 type galaxies and inside that AGN exists.
   We propose to detect its AGN components in X-ray wave bands using
   ASCA. And this unusual property of NGC5793 may lead to solve the
   unified theory between Quasars and Seyferts.
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