Results 81 to 90 of about 2,662,849 (293)
Distribution and Evolution of Metals in the Magneticum Simulations
Metals are ideal tracers of the baryonic cycle within halos. Their composition is a fossil record connecting the evolution of the various stellar components of galaxies to the interaction with the environment by in- and out-flows.
Klaus Dolag +2 more
doaj +1 more source
SZ–X-Ray Surface Brightness Fluctuations in the SPT-XMM Clusters
The hot plasma in galaxy clusters, the intracluster medium, is expected to be shaped by subsonic turbulent motions, which are key for heating, cooling, and transport mechanisms.
Charles E. Romero +12 more
doaj +1 more source
GeV Gamma-ray Flux Upper Limits from Clusters of Galaxies [PDF]
The detection of diffuse radio emission associated with clusters of galaxies indicates populations of relativistic leptons infusing the intracluster medium.
Ackermann, M. +168 more
core +3 more sources
The metallicity of the intracluster medium over cosmic time: further evidence for early enrichment [PDF]
We use Chandra X-ray data to measure the metallicity of the intracluster medium (ICM) in 245 massive galaxy clusters selected from X-ray and Sunyaev-Zel'dovich (SZ) effect surveys, spanning redshifts 0 < z < 1.2.
A. Mantz +10 more
semanticscholar +1 more source
Multiscale analysis of turbulence evolution in the density-stratified intracluster medium [PDF]
The diffuse hot medium inside clusters of galaxies typically exhibits turbulent motions whose amplitude increases with radius, as revealed by cosmological hydrodynamical simulations. However, its physical origin remains unclear. It could either be due to
Xun Shi, D. Nagai, E. Lau
semanticscholar +1 more source
IDLB: An SDN‐Based Load‐Balancing Routing Protocol for Autonomous Satellite Constellation Networks
ABSTRACT Routing in satellite constellation networks with intersatellite links has become an important aspect to enable broadband Internet access and to integrate into terrestrial networks. However, their dynamic characteristics and large physical size require specifically tailored solutions.
Manuel M. H. Roth +4 more
wiley +1 more source
We use the first eROSITA all-sky survey to investigate the contributions of active galactic nuclei (AGN) and extended gas to the total X-ray luminosity ( L _X ) of galaxy groups with different halo masses ( M _h ) at different redshifts.
Yun-Liang Zheng +12 more
doaj +1 more source
Deep Synoptic Array Science: Two Fast Radio Burst Sources in Massive Galaxy Clusters
The hot gas that constitutes the intracluster medium (ICM) has been studied at X-ray and millimeter/submillimeter wavelengths (Sunyaev–Zel’dovich effect) for decades.
Liam Connor +24 more
doaj +1 more source
Modified Entropy Models for the Intracluster Medium
Accepted to ApJ (24 pages, 31 figures)
Voit, G. Mark +3 more
openaire +2 more sources
The ‘FRIENDS for Life’ emotional health programme: Differential impact for those at risk
Abstract Background Evidence suggests that FRIENDS, a universal cognitive behavioural programme for schools, can improve children's emotional health, yet debate persists regarding its efficacy with respect to prevention versus treatment, particularly for children at risk of anxiety disorders.
Michael Wigelsworth +3 more
wiley +1 more source

