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   PR # 12224
     We propose to observe the Seyfert 1 galaxy 3C120 in order to detect
    possible emission lines in its spectrum. Since 3C120 shows some
    blazar characteristics,the search for spectral features has important
    implications for models of AGN.If beamed and isotropic components
    co-exist in this object, the strength of the emission lines allows us
    to estimate their relative contributions. The excellent spectral
    resolution of the ASCA satellite offers a unique possibility to
    quantify the blazar and thermal components in the 3C120 X-ray
    spectrum.



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