Sloshing Motions in Abell 3571 Revealed by XRISM/Resolve Velocity Mapping
Itsuki Aihara, Congyao Zhang, Sora Nakajima, Kyoko Matsushita, Hannah McCall, Irina Zhuravleva, Shogo B. Kobayashi, Kotaro Fukushima, William R. Forman, Christine Jones, Annie Heinrich, Daniele Rogantini, Kosuke Sato, Kazunori Suda, Ildar Khabibullin
astro-ph.HE
Submitted: 2026-06-29
Comments: Submitted to AAS Journal. 10 pages, 4 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Disentangling AGN Feedback and Sloshing in the Perseus Cluster with XRISM: Insights from Simulations
- The major cluster merger in Abell 2034 as seen by XRISM: Strong turbulence and spectral anomalies?
- A High Resolution Picture of the Intracluster Gas
- Bulk and turbulent gas motions in the interacting galaxy cluster Abell 3395 South observed with XRISM
- A Minimalist Merger Interpretation of XRISM's Gas Velocity Measurements in the Coma Cluster
- The X-ray properties and structure of A3571 up to $R_{500}$
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