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   61172
   The study of metal abundances in intracluster medium (ICM) is important
   for chemical evolution of the ICM. Recent ASCA observations found that
   both type-II (SNe II) and type-Ia (SNe Ia) supernovae contribute to
   metals in the ICM significantly, and it is suggested that most Si came
   from SNe II. Due to uncertainties of predicted metal yield, the origin
   of Fe is not constrained well. On the other hand, ASCA found that there
   is a large scale abundance gradient in AWM7 cluster. This indicates
   that most Fe stay around galaxies and suggests that Fe is supplied
   mildly through SNe Ia. To confirm this, we propose to observe compact
   galaxy groups HCG62, whose galaxies locate only at the central region.
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