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The Enrichment of the Intracluster Medium [PDF]

open access: yesSymposium - International Astronomical Union, 1996
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

Inferences from Surface Brightness Fluctuations of Zwicky 3146 via the Sunyaev–Zel’dovich Effect and X-Ray Observations

open access: yesThe Astrophysical Journal, 2023
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]

open access: yesThe Astrophysical Journal, 2009
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

open access: yesThe Astrophysical Journal, 2023
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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
7 pages, 1 ...
Sadhukhan, Shubhadeep   +2 more
openaire   +2 more sources

A Heating Mechanism via Magnetic Pumping in the Intracluster Medium

open access: yesThe Astrophysical Journal, 2023
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

open access: yes, 2022
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

open access: yesThe Astrophysical Journal, 2023
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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2000
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

open access: yesThe Astrophysical Journal, 2023
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

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