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• W2801432906 abstract "Recent Chandra X-ray observations of many galaxy clusters find evidence for hot metal-rich outflows preferentially aligned with the large-scale axes of X-ray cavities with typical outflow masses of around 109–1010M⊙. Here, we perform a suite of three hydrodynamic simulations to investigate if AGN jets could drive these metal-rich outflows in a representative cluster. By using both the tracer variable and virtual particle methods, and additionally following the gas metallicity evolution, we show that metal-rich gas initially located in central regions can indeed be uplifted by the AGN bubble to large distances, a phenomenon called Darwin drift in fluid mechanics, and forming a filamentary trailing outflow extending beyond 100 kpc behind the bubble. The gas entrained in the trailing outflow is entirely outflowing with an average outflow rate of nearly 100M⊙ yr−1 during the first 100 Myr, and at later times, a growing lower part flows back towards the cluster center due to gravity. The outflow mass rises up to about 1010M⊙ with an entrained iron mass of about 106–107M⊙, consistent with observations and predictions from the drift model. By the end of our simulation (∼800 Myr after the AGN event), several 109M⊙ of the uplifted high-metallicity gas still remains at large altitudes, potentially contributing to the enrichment of the bulk ICM and the broadening of central metallicity peaks observed in cool-core clusters." @default.
• W2801432906 created "2018-05-17" @default.
• W2801432906 creator A5049893166 @default.
• W2801432906 creator A5050912053 @default.
• W2801432906 date "2018-07-11" @default.
• W2801432906 modified "2023-09-23" @default.
• W2801432906 title "Metal-rich Trailing Outflows Uplifted by AGN Bubbles in Galaxy Clusters" @default.
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• W2801432906 doi "https://doi.org/10.3847/1538-4357/aac9ba" @default.
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