Results 1 to 10 of about 2,162 (186)
The Enrichment of the Intracluster Medium [PDF]
Recent observational evidence for steep dwarf galaxy luminosity functions in several rich clusters has led to speculation that their precursors, via supernovae (SNe)-driven galactic winds, may be the source of the majority of gas and metals inferred from intracluster medium (ICM) x-ray observations (Trentham 1994).
B. K. Gibson, F. Matteucci
openaire +4 more sources
The galaxy cluster Zwicky 3146 is a sloshing cool-core cluster at z = 0.291 that in Sunyaev–Zel’dovich (SZ) imaging does not appear to exhibit significant pressure substructure in the intracluster medium.
Charles E. Romero +18 more
doaj +1 more source
THE ENRICHMENT OF THE INTRACLUSTER MEDIUM [PDF]
To determine the relative contributions of galactic and intracluster stars to the enrichment of the intracluster medium (ICM), we present X-ray surface brightness, temperature, and Fe abundance profiles for a set of twelve galaxy clusters for which we have extensive optical photometry.
Sivanandam, Suresh +4 more
openaire +2 more sources
CHANDRA X-Ray Observations of A119: Cold Fronts and a Shock in an Evolved Off-axis Merger
We present Chandra X-ray observations of the dynamically complex galaxy cluster A119 ( z = 0.044). A119 is host to two narrow-angle-tail (NAT) radio sources (0053-015 and 0053-016), whose tails are oriented parallel to each other, despite orthogonally ...
Courtney B. Watson +6 more
doaj +1 more source
On the helium fingers in the intracluster medium [PDF]
7 pages, 1 ...
Sadhukhan, Shubhadeep +2 more
openaire +2 more sources
A Heating Mechanism via Magnetic Pumping in the Intracluster Medium
Turbulence driven by active galactic nuclei activity, cluster mergers, and galaxy motion constitutes an attractive energy source for heating the intracluster medium (ICM).
Francisco Ley +5 more
doaj +1 more source
Plasma Physics of the Intracluster Medium
This Chapter provides a brief tutorial on some aspects of plasma physics that are fundamental to understanding the dynamics and energetics of the intracluster medium (ICM). The tutorial is split into two parts: one that focuses on the thermal plasma component -- its stability, viscosity, conductivity, and ability to amplify magnetic fields to dynamical
Kunz, Matthew W. +2 more
openaire +2 more sources
Mirror Acceleration of Cosmic Rays in a High-β Medium
In a weakly compressible high- β medium, pitch-angle scattering and the associated scattering acceleration of cosmic rays (CRs) by anisotropic Alfvén and slow modes of magnetohydrodynamic (MHD) turbulence is inefficient.
Alex Lazarian, Siyao Xu
doaj +1 more source
A multiphase model for the intracluster medium [PDF]
Nine pages, submitted to Monthly Notices of the RAS.
Nagai, Daisuke +2 more
openaire +3 more sources
Electron Reacceleration via Ion Cyclotron Waves in the Intracluster Medium
In galaxy clusters, the intracluster medium (ICM) is expected to host a diffuse, long-lived, and invisible population of “fossil” cosmic-ray electrons (CRe) with 1–100 MeV energies.
Aaron Tran +4 more
doaj +1 more source

