XRISM velocity maps of Abell 3571 show subsonic gas motions and thermodynamic asymmetry consistent with early-phase sloshing from an off-axis minor merger with Abell 3572 as candidate perturber.
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7 Pith papers cite this work. Polarity classification is still indexing.
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Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
XRISM measurements indicate turbulent dissipation from jets struggles to balance cooling in cluster atmospheres except possibly in limited inner regions of systems like Hydra A.
Cosmological simulations with AGN jet feedback reproduce observed cool-core cluster ICM properties more accurately than isolated simulations or IllustrisTNG due to merger-driven effects on gas velocity and warm gas abundance.
citing papers explorer
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Sloshing Motions in Abell 3571 Revealed by XRISM/Resolve Velocity Mapping
XRISM velocity maps of Abell 3571 show subsonic gas motions and thermodynamic asymmetry consistent with early-phase sloshing from an off-axis minor merger with Abell 3572 as candidate perturber.
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Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster
Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.
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The Quiescent Sloshing Core of Abell 496 with XRISM
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
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Are X-ray Atmospheres Heated by Turbulent Dissipation? XRISM Constraints
XRISM measurements indicate turbulent dissipation from jets struggles to balance cooling in cluster atmospheres except possibly in limited inner regions of systems like Hydra A.
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Active galactic nucleus driven jet feedback in cosmologically forming cool-core galaxy clusters I: The effect of hierarchical assembly on intra-cluster medium properties
Cosmological simulations with AGN jet feedback reproduce observed cool-core cluster ICM properties more accurately than isolated simulations or IllustrisTNG due to merger-driven effects on gas velocity and warm gas abundance.
- Suppression of Radiative Cooling in Galaxy Cluster Cores by the Combination of AGN Heating and Sloshing
- A Comprehensive Study of Morphology and Kinematics in Extended Nebulae Around UV Luminous Quasars at $z\approx1$