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1 Introduction
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2 Gas and metal in the ICM: Previous studies
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3 A non-standard IMF
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4 Global cluster results: The monolithic approach
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5 A chemical model for the ICM evolution
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6 A fiducial model
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7 Varying the Galaxy Formation History
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8 Choosing the IMF "ad hoc''
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9 Abundance ratios in the ICM
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10 Summary and conclusions
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References
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