Results 181 to 190 of about 2,662,849 (293)
Modern radio telescopes are revolutionising our understanding of non-thermal phenomena in galaxy clusters, collecting large samples of extended sources with unprecedented sensitivity and angular resolution.
Balboni M. +20 more
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The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters [PDF]
Folkert S J Nobels +4 more
openalex +1 more source
Chemical Composition of the Intracluster Medium
Clusters of galaxies are massive enough to be considered representative samples of the Universe, and to retain all of the heavy elements synthesized in their constituent stars. Since most of these metals reside in hot plasma, X-ray spectroscopy of clusters provides a unique and fundamental tool for studying chemical evolution.
openaire +2 more sources
We present a detailed study of cool-core systems in a sample of four galaxy clusters (RXCJ1504.1-0248, A3112, A4059, and A478) using archival X-ray data from the Chandra X-ray Observatory.
FanLam Ng, Shutaro Ueda
doaj +1 more source
Energetics of Jet Interactions with the Intracluster Medium [PDF]
J. H. Beall +4 more
openalex +1 more source
A Yin-yang Galaxy Cluster Merger in A1914 Revealed by XRISM
Hierarchical mergers of galaxy clusters play a key role in converting gravitational energy into thermal and kinetic energy in the local Universe.
Annie Heinrich +6 more
doaj +1 more source
The merger history of clusters and its effect on the X-ray properties of the intracluster medium [PDF]
David R. Rowley, P. Thomas, Scott T. Kay
openalex +1 more source
Galaxy clusters, the largest gravitationally bound structures, host a hot, diffuse plasma with poorly understood viscosity and magnetic field amplification.
S. Adduci Faria +2 more
doaj +1 more source
Observations of magnetic fields in intracluster medium [PDF]
F. Govoni
openalex +1 more source
SPT-CL J0417–4748: A Deep Chandra Study of a Relaxed Galaxy Cluster without Central Star Formation
We present an in-depth Chandra X-ray analysis of the galaxy cluster SPT-CL J0417−4748 (hereafter SPT J0417) at z = 0.58 with a focus on its thermodynamic properties and the apparent absence of central star formation. Utilizing a total Chandra exposure of
Taweewat Somboonpanyakul +9 more
doaj +1 more source

