tokens: The authors are very thankful to the referee for valuable comments that helped to improve the paper. The authors would also like to thank Jesper Rasmussen and Alastair Sanderson for kindly providing their observational data, as well as Susana Planelles and Elena Rasia for kindly providing their simulation outputs and for useful discussions. This work is partly based on the XMM-Newton AO-12 proposal “The XMM-Newton view of chemical enrichment in bright galaxy clusters and groups” (PI: de Plaa), and is a part of the CHEERS (CHEmical Evolution Rgs cluster Sample) collaboration. H.A. acknowledges the support of NWO via a Veni grant. P.K. acknowledges financial support from STFC. C.P. acknowledges support from ERC Advanced Grant Feedback 340442. T.H.R. acknowledges support from the DFG through grant RE 1462/6 and through the Transregional Collaborative Research Centre TRR33 The Dark Universe, project B18. This project has been supported by the Lendület LP2016-11 grant awarded by the Hungarian Academy of Sciences. This work is based on observations obtained with XMM-Newton , an ESA science mission with instruments and contributions directly funded by ESA member states and the USA (NASA). The SRON Netherlands Institute for Space Research is supported financially by NWO, The Netherlands Organisation for Scientific Research.
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