******************************************************                         
    PR # 31244                                                                   
     We propose to two compact galaxy groups HCG48, HCG42 that were omitte       
     d at AO-1. HCG62 observation of adopted our proposal detected diffuse       
      X-ray emission as ROSAT. The best fit value of Raymond-Smith is temp       
     erature of 0.85 keV and abundance of 0.17 solar. But, we discovered s       
     trong Argon line emission for best fit model. It is possible to low a       
     bundance because of other reason. Heavy elements will be disappears i       
     n dust and only Argon of rare gases can be seen in diffuse hot gas. A       
     rgon line emission rate was unclear in HCG62 observation. We should o       
     bserve new bright same galaxy groups that is  secured positive eviden       
     ce. So we propose this target that be expected with strong diffuse em       
     ission.                                                                     
                                                                                 
  ******************************************************