Results 121 to 130 of about 2,373,370 (260)
Two-Temperature Intracluster Medium in Merging Clusters of Galaxies
, 1999 We investigate the evolution of intracluster medium during a cluster merger, explicitly considering the relaxation process between the ions and electrons by N-body and hydrodynamical simulations.
Edge A. C. +10 more
core +2 more sources
The Fate of Asymptotic Giant Branch Winds in Massive Galaxies and the Intracluster Medium
Astrophysical Journal, 2019 Winds from asymptotic giant branch (AGB) stars not only provide mass and energy return, but also produce dust grains in massive elliptical galaxies. Due to the fast stellar velocity, the wind is thought to form a comet-like tail, similar to Mira in the ...
Yuan Li, G. Bryan, E. Quataert
semanticscholar +1 more source
The Seeding of Cosmic Ray Electrons by Cluster Radio Galaxies: A Review
GalaxiesRadio 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
Non-Kolmogorov turbulence in multiphase intracluster medium driven by cold gas precipitation and AGN jets [PDF]
, 2021 Chaoran Wang +4 more
openalex +1 more source
Probing cluster environments of blazars through gamma-gamma absorption
, 2014 Most blazars are known to be hosted in giant elliptic galaxies, but their cluster environments have not been thoroughly investigated. Cluster environments may contain radiation fields of low-energy photons created by nearby galaxies and/or stars in the ...
Böttcher, Markus, Sushch, Iurii
core +1 more source
, 2011 Cosmological shocks are a critical part of large-scale structure formation, and are responsible for heating the intracluster medium in galaxy clusters. In addition, they are also capable of accelerating non-thermal electrons and protons. In this work, we
Burns, Jack O. +5 more
core +1 more source
Redshift Evolution in the Iron Abundance of the Intracluster Medium
, 2009 Clusters of galaxies provide a closed box within which one can determine the chemical evolution of the gaseous baryons with cosmic time. We studied this metallicity evolution in the hot X-ray emitting baryons through an analysis of XMM-Newton ...
Arnaud +15 more
core +1 more source
Merger Shocks Enhance Quenching in Local Galaxy Clusters
The Astrophysical JournalWe 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
doaj +1 more source
On viscosity, conduction and sound waves in the intracluster medium
, 2005 Recent X-ray and optical observations of the Perseus cluster indicate that the viscous and conductive dissipation of sound waves is the mechanism responsible for heating the intracluster medium and thus balancing radiative cooling of cluster cores.
A. C. Fabian +53 more
core +4 more sources