The Halo Mass–Temperature Relation for Clusters, Groups, and Galaxies [PDF]
Iu. Babyk, B. R. McNamara
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Luminosity segregation in galaxy clusters as an indication of dynamical evolution [PDF]
Theoretical models describing the dynamical evolution of self-gravitating systems predict a spatial mass segregation for more evolved systems, with the more massive objects concentrated toward the center of the configuration. From the observational point
Baier, F. W., Schmidt, K.-H.
core +1 more source
Exploiting Machine Learning and Disequilibrium in Galaxy Clusters to Obtain a Mass Profile
We use 3D k -means clustering to characterize galaxy substructure in the A2146 cluster of galaxies ( z = 0.2343). This method objectively characterizes the cluster’s substructure using projected position and velocity data for 67 galaxies within a 2.305 ...
Mark J. Henriksen, Prajwal Panda
doaj +1 more source
Mechanical feedback from active galactic nuclei in galaxies, groups and clusters [PDF]
B. R. McNamara, P. E. J. Nulsen
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Formation Channels of Diffuse Lights in Groups and Clusters over Time
We explore the formation of the intragroup light and intracluster light, representing diffuse lights within groups and clusters, from the point that z = 1.5.
Kyungwon Chun +4 more
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The environmental history of group and cluster galaxies in a Λ cold dark matter universe [PDF]
G. De Lucia +4 more
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Galaxy Cluster Constraints on Extensions of Modified Gravity
Modified Newtonian dynamics (MOND) has achieved notable success in explaining galaxy-scale phenomena and has made several unexpected, a priori predictions that align with observations.
E. C. Diggins, D. R. Wik
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The splashback radius of groups and clusters of galaxies at low redshifts [PDF]
Ф. Г. Копылова +1 more
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The Stellar Population and Star Clusters in the Unusual Local Group Galaxy IC 10
Deidre A. Hunter
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The baryon budget on the galaxy group/cluster boundary [PDF]
Alastair J. R. Sanderson +6 more
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