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Enrichment of the Hot Intracluster Medium: Numerical Simulations
Space Science Reviews, 2018The distribution of chemical elements in the hot intracluster medium (ICM) retains valuable information about the enrichment and star formation histories of galaxy clusters, and on the feedback and dynamical processes driving the evolution of the cosmic ...
V. Biffi +3 more
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Nonlinear dynamo in the intracluster medium
Classical and Quantum Gravity, 2018Abstract Hot plasma in galaxy clusters, the intracluster medium is observed to be magnetized with magnetic fields of around a μ G and the correlation scales of tens of kiloparsecs, the largest scales of the magnetic field so far observed in the Universe.
Andrey Beresnyak, Francesco Miniati
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Chemical enrichment of the Intracluster Medium
Astronomische Nachrichten, 2005X-ray observations (e.g. Fukazawa et al. 1998) show that the Intracluster Medium (ICM) contains metals with abundances ~ 0.2 - 0.3 Z ⊙. Since heavy elements are produced mainly in stars of cluster galaxies, they must have been transported into the intracluster space.
Baumgartner, Verena +1 more
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Imaging the Hot Intracluster Medium
1992Clusters of galaxies contain large amounts of hot, diffuse x—ray emitting gas. Observations of this gas can be used to measure the gas mass, the cluster virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and ...
C. Jones, W. Forman
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Evolution of Clusters and the Intracluster Medium
1993I review observations and theoretical models of evolution of gas in clusters of galaxies. The mass of hot gas is an important component of clusters of galaxies, equalling or exceeding the total mass in galaxies in most clusters. The hot gas also traces the gravitational potential of the cluster, giving better measurements of the total mass of a cluster
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The velocity structure of the intracluster medium of the Centaurus cluster
Monthly Notices of the Royal Astronomical Society, 2022Efrain Gatuzz +2 more
exaly
An H α/X-ray orphan cloud as a signpost of intracluster medium clumping
Monthly Notices of the Royal Astronomical Society, 2021Chong Ge, Rongxin Luo, M Sun
exaly