Results 61 to 70 of about 2,500,510 (339)
Models of ram-pressure stripping and some extra discussion added, references added. Conclusions unchanged. 20 pages, 15 figures. Accepted for publication in MNRAS.
Weinmann Simone M. +3 more
openaire +3 more sources
THE ELLIPTICITIES OF GALAXIES IN GALAXY CLUSTERS OF DIFFERENT MORPHOLOGICAL TYPE
The distribution of galaxy ellipticities was analyzed for 207 rich PF galaxy clusters found in the Munster Red Sky Survey Galaxy Catalogue. Clusters with BM types from a comparison with the ACO catalogue were also classified on the new scheme.
E. A. Panko, P. Flin
doaj +1 more source
Simulating the formation of a proto-cluster at z~2
We present results from two high-resolution hydrodynamical simulations of proto-cluster regions at z~2.1. The simulations have been compared to observational results for the socalled Spiderweb galaxy system, the core of a putative proto-cluster region at
Borgani, S. +5 more
core +1 more source
Constraining galaxy cluster temperatures and redshifts with eROSITA survey data [PDF]
Context. The nature of dark energy is imprinted in the large-scale structure of the Universe and thus in the mass and redshift distribution of galaxy clusters.
K. Borm +3 more
semanticscholar +1 more source
Constructing a Galaxy Cluster Catalog in IllustrisTNG300 Using the Mulguisin Algorithm
We present a new simulated galaxy cluster catalog based on the IllustrisTNG simulation. We use the Mulguisin (MGS) algorithm to identify galaxy overdensities.
Lael Shin +4 more
doaj +1 more source
Probing the evolution of galaxy clusters using SZ effect and non-thermal emission: First results from A1413 [PDF]
Mass is the most fundamental property of galaxy clusters. However, measuring it is still a challenge. Calibrating mass from intracluster medium observables such as the Sunyaev-Zel’dovich (SZ) effect is subject to uncertainty and biases because of the ...
Pachchigar M., Perrott Y., Parashar T.
doaj +1 more source
Galactic cannibalism and CDM density profiles [PDF]
Using N-body simulations we show that the process of formation of the brightest cluster galaxy through dissipationless galactic cannibalism can affect the inner cluster dark matter density profile.
Barnes +48 more
core +2 more sources
Characterising superclusters with the galaxy cluster distribution [PDF]
G. Chon, et al., “Characterising superclusters with the galaxy cluster distribution”, Astronomy & Astrophysics, Vol. 567, August 2014. This version of record is available at: https://www.aanda.org/articles/aa/abs/2014/07/aa24047-14/aa24047-14.html ...
G. Chon +3 more
semanticscholar +1 more source
Clustering of Submillimetre-Selected Galaxies [PDF]
Using accurate positions from very deep radio observations to guide multi-object Keck spectroscopy, we have determined a substantially complete redshift distribution for very luminous, distant submillimeter(submm)-selected galaxies (SMGs). A sample of 73 redshifts for SMGs in 7 fields contains a surprisingly large number of `associations': systems of ...
Blain, Andrew W. +3 more
openaire +2 more sources
A fully flexible ion‐gel‐gated graphene‐channel transistor driven by a triboelectric nanogenerator enables self‐powered tactile sensing and synaptic learning. Mimicking spike‐rate‐dependent plasticity, the device exhibits frequency‐selective potentiation and depression, supporting rate‐coded neuromorphic computation even under flex.
Hanseong Cho +3 more
wiley +1 more source

