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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Stacking analysis of eROSITA observations detects statistically significant X-ray signal from hot gas out to 2 r_200m with a transition at the halo boundary, showing higher gas spread than in IllustrisTNG simulations.
Stacking analysis yields L-M slope 1.56, slightly steeper than self-similar, with X-ray detected clusters showing more centrally concentrated profiles than undetected ones.
citing papers explorer
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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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The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
Stacking analysis of eROSITA observations detects statistically significant X-ray signal from hot gas out to 2 r_200m with a transition at the halo boundary, showing higher gas spread than in IllustrisTNG simulations.
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The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
Stacking analysis yields L-M slope 1.56, slightly steeper than self-similar, with X-ray detected clusters showing more centrally concentrated profiles than undetected ones.