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   PR # 22186
    Spatially resolved ASCA SIS/GIS spectra of intracluster gas will be  
    used to determine the radial distribution of metal abundances in the 
    outer parts of two clusters with redshifts z = 0.1-0.15.  At this    
    distance, nearly all of the cluster emission should fit in the SIS   
    field of view.  These particular clusters are bright enough that it  
    should still be possible to spatially resolve the metal abundances   
    in their outer parts in order to discriminate between various metal  
    injection models for the contamination of intracluster gas.          
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