Results 181 to 190 of about 16,803 (214)

Effectiveness of a Web-Based Self-Guided Intervention (MINDxYOU) for Reducing Stress and Promoting Mental Health Among Health Professionals: Results From a Stepped-Wedge Cluster Randomized Trial.

J Med Internet Res
López-Del-Hoyo Y, Fernández-Martínez S, Perez-Aranda A, Monreal-Bartolomé A, Barceló-Soler A, Camarero-Grados L, Armas-Landaeta C, Guzmán-Parra J, Carbonell V, Campos D, Chen X, García-Campayo J.   +11 more
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Metals in the intracluster medium

AIP Conference Proceedings, 2012
We 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, Kosuke Sato, Eri Sakuma, Takayuki Tamura   +3 more
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Turbulence in the Intracluster Medium

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.
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The Intracluster Medium

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.
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Chemical enrichment of the Intracluster Medium

Astronomische Nachrichten, 2005
X-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, Breitschwerdt, Dieter   +1 more
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Imaging the Hot Intracluster Medium

1992
Clusters 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

1993
I 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, 2022
Efrain Gatuzz, Jeremy Sanders, Andrew C Fabian   +2 more
exaly  

Witnessing the intracluster medium assembly at the cosmic noon in JKCS 041

Monthly Notices of the Royal Astronomical Society, 2023
Stefano Andreon, Simon R Dicker, Brian S Mason   +2 more
exaly