  We investigate efficiency and time dependence of metal enrichment processes
in the Intra-Cluster Medium (ICM). In this presentation we concentrate on the
effects of galactic winds. The mass loss rates due to galactic winds are
calculated with a special algorithm, which takes into account cosmic rays and
magnetic fields. This algorithm is embedded in a combined N-body/hydrodynamic
code which calculates the dynamics and evolution of a cluster. We present mass
loss rates depending on galaxy properties like type, mass, gas mass fraction
and the surrounding ICM. In addition we show metallicity maps as they would be
observed with X-ray telescopes.
