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Formation of a low-mass galaxy from star clusters in a 600-million-year-old Universe
NatureGael Noirot +2 more
exaly
Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang
NatureA Adamo, E Vanzella, J M Diego
exaly
Scaling Properties of Galaxy Groups [PDF]
Galaxy groups and poor clusters are more common than rich clusters, and host the largest fraction of matter content in the Universe. Hence, their studies are key to understand the gravitational and thermal evolution of the bulk of the cosmic matter ...
Lorenzo Lovisari +3 more
doaj +3 more sources
Accretion of galaxy groups into galaxy clusters [PDF]
We study the role of group infall in the assembly and dynamics of galaxy clusters in ΛCDM. We select 10 clusters with virial mass M200 ∼1014 M from the cosmological hydrodynamical simulation Illustris and follow their galaxies with stellar mass M⊙ ≥ 1.5 ×
Benavides, José A. +2 more
core +5 more sources
THE PECULIARITIES IN O-TYPE GALAXY CLUSTERS
We present the results of analysis of 2D distribution of galaxies in galaxy cluster fields. The Catalogue of Galaxy Clusters and Groups PF (Panko & Flin) was used as input observational data set.
E. A. Panko, S. I. Emelyanov
doaj +2 more sources
Galaxy Evolution in Groups and Clusters [PDF]
In this thesis, we investigate the extent to which galaxy evolution is driven by processes common to the group and cluster environments. A bimodality of galaxy properties such as star formation, strongly dependent upon the local overdensity of galaxies ...
Wilman, David John
core +2 more sources
Constraints on the Optical Depth of Galaxy Groups and Clusters [PDF]
Future data from galaxy redshift surveys, combined with high-resolutions maps of the cosmic microwave background, will enable measurements of the pairwise kinematic Sunyaev–Zel'dovich (kSZ) signal with unprecedented statistical significance.
Daisuke Nagai +5 more
core +5 more sources
Properties of Fossil Groups of Galaxies
We review the formation and evolution of fossil groups and clusters from both the theoretical and the observational points of view. In the optical band, these systems are dominated by the light of the central galaxy.
J. Alfonso L. Aguerri, Stefano Zarattini
doaj +1 more source
The Effect of Splashback on Weak Lensing Mass Estimates of Galaxy Clusters and Groups
The splashback radius of a dark matter halo, which corresponds to the first apocenter radius reached by infalling matter and substructures, has been detected around galaxy clusters using a multitude of observational methods, including weak lensing ...
Yuanyuan Zhang +5 more
doaj +2 more sources
The 2dF Galaxy Redshift Survey: the clustering of galaxy groups [PDF]
16 pages.
Padilla, Nelson D. +29 more
openaire +8 more sources

