The full iron budget in simulated galaxy clusters: The chemistry between gas and stars

Open Access

Fig. 1.

Iron share between ICM and stellar component as a function of the total system mass. On both axes, the quantities are computed either within R₅₀₀ (blue asterisks) or within R₂₀₀ (red diamonds). The two lines correspond to the linear best fit of the two datasets in log-log space.

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