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- W2624366129 abstract "Suzaku measurements of a homogeneous metal distribution of $Zsim0.3$ Solar in the outskirts of the nearby Perseus cluster suggest that chemical elements were deposited and mixed into the intergalactic medium before clusters formed, likely over 10 billion years ago. A key prediction of this early enrichment scenario is that the intracluster medium in all massive clusters should be uniformly enriched to a similar level. Here, we confirm this prediction by determining the iron abundances in the outskirts ($r>0.25r_{200}$) of a sample of ten other nearby galaxy clusters observed with Suzaku for which robust measurements based on the Fe-K lines can be made. Across our sample the iron abundances are consistent with a constant value, $Z_{rm Fe}=0.316pm0.012$ Solar ($chi^2=28.85$ for 25 degrees of freedom). This is remarkably similar to the measurements for the Perseus cluster of $Z_{rm Fe}=0.314pm0.012$ Solar, using the Solar abundance scale of Asplund et al. (2009)." @default.
- W2624366129 created "2017-06-15" @default.
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- W2624366129 date "2017-06-20" @default.
- W2624366129 modified "2023-10-10" @default.
- W2624366129 title "A uniform metallicity in the outskirts of massive, nearby galaxy clusters" @default.
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- W2624366129 doi "https://doi.org/10.1093/mnras/stx1542" @default.
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