Results 101 to 110 of about 1,040 (235)
Correlations in Relaxed Clusters of Galaxies
The correlations among different quantities in galaxy clusters, observed by Newman et al. (2013a,b), are investigated. We find an anti-correlation among the slope α, the effective radius, Re, and a correlation among the core radius rcore and Re. Moreover,
Babyk Iu., Del Popolo A.
doaj +1 more source
We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM).
Arsen Levitskiy +4 more
doaj +1 more source
We present a selection of candidates of clusters and protoclusters of galaxies identified in the photometric data of the HSC-SSP Wide Public Data Release 3 (PDR3), spanning the redshift range 0.1 ≤ z ≤ 2. The selection method, detailed in Vicentin et al.,
Marcelo C. Vicentin +4 more
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Intracluster Light in Nearby Galaxy Clusters: Relationship to the Halos of Brightest Cluster Galaxies [PDF]
Anthony H. Gonzalez +2 more
openalex +1 more source
Star formation activities in early-type brightest cluster galaxies [PDF]
F. S. Liu, Shude Mao, X. M. Meng
openalex +1 more source
Detection of Compton Scattering in the Jet of 3C 84
3C 84 is the brightest cluster galaxy in the Perseus Cluster. It is among the closest radio-loud active galaxies and among the very few that can be detected from low-frequency radio up to TeV γ -rays.
Ioannis Liodakis +79 more
doaj +1 more source
The K-Band Hubble Diagram for X-Ray Selected Brightest Cluster Galaxies [PDF]
Robert G. Mann, C. A. Collins
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The Manhattan Suite: Accelerated Galaxy Evolution in the Early Universe
Observational advances have allowed the detection of galaxies, protoclusters, and galaxy clusters at higher and higher redshifts, opening a new view into extreme galaxy evolution.
Douglas Rennehan
doaj +1 more source
JWST Photometry of Globular Cluster Populations in MACS0417.5−1154
Deep JWST imaging of the massive galaxy cluster MACS0417.5−1154, at redshift z = 0.443, reveals a huge population of globular clusters (GCs) and ultracompact dwarfs (UCDs) primarily distributed around its single central giant brightest cluster galaxy ...
William E. Harris +10 more
doaj +1 more source
Sersic 159-03: Discovery of the Brightest Soft X-Ray Excess Emitting Cluster of Galaxies [PDF]
Massimiliano Bonamente +2 more
openalex +1 more source

