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    PR # 31219                                                                   
     We propose the observation of two clusters of galaxies, Klemola44 and       
      A644, to check our interpretation for the cool component which is se       
     en at the center of the clusters. We have an idea that the cool compo       
     nent is ISM of cD galaxy rather than the product of radiative cooling       
     .                                                                           
                                                                                 
                                                                                 
                                                                                 
                                                                                 
                                                                                 
                                                                                 
                                                                                 
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