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   PR # 22146
    We propose to obtain a broad band X-ray spectrum with good statistics
    of Seyfert 1.9 galaxy ESO103-G35, one of the few Seyfert's observed  
    to have a large, variable absorption column. Based on non-simultan-  
    eous Ginga & ROSAT observations, we expect to find a heavily absorbed
    spectrum in the hard X-rays and a soft component. Spectral and       
    temporal analysis will allow us to determine whether this object more
    resembles a Seyfert 2, with scattered or extended soft emission, or a
    Seyfert 1with a warm absorber.  Study of this transition object will 
    allow us to test the assertion that heavily absorbed Seyfert 1's are 
    obscured bythe molecular torus as Seyfert 2's are assumed to be.     
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