Results 51 to 60 of about 2,230 (139)
The three-dimensional shapes of the galaxy cluster intracluster medium in eRASS1
Aims. The three-dimensional shapes of clusters are important for understanding the astrophysics of the clusters and as a probe in cosmological studies. Methods. We estimate the most probable three-dimensional shape of galaxy clusters in the first eROSITA
Kulkarni S. +4 more
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The Seeding of Cosmic Ray Electrons by Cluster Radio Galaxies: A Review
Radio galaxies in clusters of galaxies are a prominent reservoir of magnetic fields and of non-thermal particles, which become mixed with the intracluster medium.
Franco Vazza, Andrea Botteon
doaj +1 more source
Merger Shocks Enhance Quenching in Local Galaxy Clusters
We report evidence for enhanced quenching in low-redshift galaxy clusters hosting radio relics. This effect is strongest for low-mass galaxies and is consistent with a rapid quenching of star formation.
Ian D. Roberts
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Investigating the Intracluster Medium Viscosity Using the Tails of GASP Jellyfish Galaxies
The microphysics of the intracluster medium (ICM) in galaxy clusters is still poorly understood. Observational evidence suggests that the effective viscosity is suppressed by plasma instabilities that reduce the mean free path of particles. Measuring the
Alessandro Ignesti +15 more
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XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029
We present XRISM Resolve observations of the core of the hot, relaxed galaxy cluster Abell 2029 (A2029). We find that the line-of-sight bulk velocity of the intracluster medium (ICM) within the central 180 kpc is at rest with respect to the brightest ...
XRISM Collaboration +138 more
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Intensity Fluctuations of Radio Halos in Galaxy Clusters: Insights from Power Spectrum Estimation
Nonthermal synchrotron emissions from radio halos allow us to study mechanisms of particle (re)acceleration, magnetic field distribution, merger history, and turbulence in the intracluster medium.
Srijita Pal +5 more
doaj +1 more source
The eROSITA Final Equatorial-Depth Survey (eFEDS)
Context. This is the second paper in a series exploring the X-ray properties of galaxy clusters optically selected by the Subaru Hyper Suprime-Cam (HSC) survey, using data from the SRG/eROSITA Final Equatorial-Depth Survey (eFEDS). Aims.
Nguyen-Dang N. T. +19 more
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We study the global kinematics of the Perseus galaxy cluster (A426) at redshift z = 0.017 using a large sample of galaxies from our new MMT/Hectospec spectroscopic observation for this cluster.
Wooseok Kang +5 more
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XRISM Observations of the Prototypical Cold Front in A3667
We present high-resolution X-ray spectroscopy of the merging galaxy cluster A3667 with XRISM/Resolve. Two observations, targeting the cluster X-ray core and the prototypical cold front, were performed with exposures of 105 and 276 ks, respectively.
Yuki Omiya +15 more
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