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   PR # 22182
    We propose ASCA spectra for three clusters of galaxies with evidence 
    for cooling flows and excess soft X-ray absorption.  The principle   
    aim is to determine the physical state and ultimate repository of the
     ~300 Msun/yr of gas cooling in these systems.  We will use emission 
    line diagnostics to derive the amount and spatial distribution of the
    cooling material, and the density distribution of inhomogeneities.   
    The presence of the excess soft X--ray absorption  will be verified, 
    and we will determine if it is intrinsic to the cluster or in the    
    foreground.  The spatial distribution of this cold material will be  
    derived.  We will also determine overall cluster properties, such as 
    the gas temperature and density profiles, the amount and distribution
   of dark matter, and the variat
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