Results 161 to 170 of about 2,187 (187)
Some of the next articles are maybe not open access.
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
openaire +1 more source
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
openaire +1 more source
The velocity structure of the intracluster medium of the Centaurus cluster
Monthly Notices of the Royal Astronomical Society, 2022Stephen Walker +2 more
exaly
Witnessing the intracluster medium assembly at the cosmic noon in JKCS 041
Monthly Notices of the Royal Astronomical Society, 2023Anand Raichoor +2 more
exaly
Turbulent pressure support and hydrostatic mass bias in the intracluster medium
Monthly Notices of the Royal Astronomical Society, 2020Dominique Eckert +2 more
exaly
An H α/X-ray orphan cloud as a signpost of intracluster medium clumping
Monthly Notices of the Royal Astronomical Society, 2021Ming Sun, Masafumi Yagi, Pavel Jachym
exaly