  Based on XMM-Newton observations of a sample of galaxy clusters, we have
measured the elemental abundances (mainly O, Si, S, and Fe) and their spatial
distributions in the intracluster medium (ICM). In the outer region of the ICM,
observations of the O:Si:S:Fe ratio are consistent with the solar value,
suggesting that the metals in the ICM were produced by a mix of supernovae
(SNe) Ia and II. On the other hand, around the cD galaxy, the O/Fe ratios are
about half of the solar value because of a central excess of the Fe abundance.
An increase of the relative contribution from SNe Ia in the cD galaxy to the
metal production towards the center is the most likely explanation.
