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   PR # 43031
   The ROSAT All Sky Survey revealed a number of IRAS galaxies with high
   X-ray luminosities. Generally they have very steep soft X-ray spectra
   and are classified optically, varyingly, as active or non-active
   galaxies. It is proposed to study two of these galaxies with ASCA in
   order to determine the relative importance of Starburst and AGN
   processes in producing the high emission levels. An AGN component may
   show up at harder X-rays, while the contribution of thermal emission
   associated with Star
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