Results 221 to 230 of about 2,679,570 (255)
Interventions for treating tibial shaft fractures in children. [PDF]
Cochrane Database Syst RevLawniczak D +3 more
europepmc +1 more source
Witnessing the intracluster medium assembly at the cosmic noon in JKCS 041 [PDF]
Monthly Notices of the Royal Astronomical Society, 2023 In this work we study the intracluster medium of a galaxy cluster at the cosmic noon: JKCS 041 at z = 1.803. A 28h long Sunyaev-Zel’dovich (SZ) observation using MUSTANG-2 allows us to detect JKCS 041 , even if intrinsically extremely faint compared to
S Andreon, Simon Dicker, B Ladjelate
exaly +4 more sources
Turbulence in the Intracluster Medium [PDF]
, 2014 We review our knowledge about turbulence in the intracluster medium, a very hot, dilute plasma that permeates clusters of galaxies. A thorough understanding of turbulence in the intracluster medium is crucial for the use of clusters to determine cosmological parameters.
Brüggen, M., Vazza, F.
openaire +2 more sources
Turbulence decay in the density-stratified intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 Turbulence evolution in a density-stratified medium differs from that of homogeneous isotropic turbulence described by the Kolmogorov picture. We evaluate the degree of this effect in the intracluster medium (ICM) with hydrodynamical simulations.
Xun Shi, Congyao Zhang, Shi Xun
exaly +3 more sources
Turbulence in stratified atmospheres: implications for the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 The gas motions in the intracluster medium (ICM) are governed by turbulence. However, since the ICM has a radial profile with the centre being denser than the outskirts, ICM turbulence is stratified.
Rajsekhar Mohapatra +2 more
exaly +2 more sources
Turbulent density and pressure fluctuations in the stratified intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 Turbulent gas motions are observed in the intracluster medium (ICM). The ICM is density-stratified, with the gas density being highest at the centre of the cluster and decreasing radially outwards.
Rajsekhar Mohapatra +2 more
exaly +2 more sources
The history of chemical enrichment in the intracluster medium from cosmological simulations [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic star formation and on the effects of different gas processes.
V Biffi, S Planelles, E Rasia
exaly +2 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Monthly notices of the Royal Astronomical Society, 2020
In the outskirts of the intracluster medium (ICM) in galaxy clusters, the temperature decreases with radius. Due to the weakly collisional nature of the plasma, these regions are susceptible to the magneto-thermal instability (MTI), which can sustain ...
Thomas Berlok +3 more
semanticscholar +1 more source
In the outskirts of the intracluster medium (ICM) in galaxy clusters, the temperature decreases with radius. Due to the weakly collisional nature of the plasma, these regions are susceptible to the magneto-thermal instability (MTI), which can sustain ...
Thomas Berlok +3 more
semanticscholar +1 more source
Metals in the intracluster medium
AIP Conference Proceedings, 2012We derived radial abundance profiles of O, Mg, Si, S and Fe in the intracluster medium (ICM) of several clusters and groups of galaxies up to about 0.3 r180 with Suzaku and those of Fe in 28 nearby brightest clusters of galaxies up to 0.3-0.5 r180 with XMM. Within 0.05 r180, Fe abundance scatters from 0.5 to 1 solar.
Kyoko Matsushita +3 more
openaire +1 more source
1992
Clusters of galaxies are full of hot, diffuse plasma, with typical temperatures and electron densities of T ~ 7x107 K and n e ~ 10-3 cm-3, This intraclustermedium (ICM) produces copious X-ray emission, and typical cluster X-ray luminositiesare L x ~ 1043 - 1045 ergs s-1.
openaire +1 more source
Clusters of galaxies are full of hot, diffuse plasma, with typical temperatures and electron densities of T ~ 7x107 K and n e ~ 10-3 cm-3, This intraclustermedium (ICM) produces copious X-ray emission, and typical cluster X-ray luminositiesare L x ~ 1043 - 1045 ergs s-1.
openaire +1 more source