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   PR # 11112
    We propose that the two most luminous galaxies found in the IRAS
    survey are observed with ASCA. Both show high excitation optical
    emission lines and a polarized continuum which suggests that they
    both contain powerful quasars. They are among the most luminous
    objects known. If there is an X-ray emitting quasar in each object
    which is not visible at other wavelengths due to obscuration then it
    should be directly detectable above a few keV where photoelectric
    absorption becomes less important.




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