2022
DOI: 10.3847/1538-4357/ac4dfb
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The Missing Metal Problem in Galaxy Clusters: Characterizing the Early Enrichment Population

Abstract: Rich and poor galaxy clusters have the same measured halo metallicity, 0.35–0.4 Z ⊙, even though they are an order of magnitude apart in stellar fraction, M */M gas. The measured intracluster medium (ICM) metallicity in high-mass clusters cannot be explained by the visible stellar population as stars typically make up 3%–20% of the total baryon mass. The independence of metallicity of M */M gas suggests an external and un… Show more

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Cited by 3 publications
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