Results 51 to 60 of about 2,267,963 (287)
Detection of a Star Forming Galaxy in the Center of a Low-Mass Galaxy Cluster
Brightest Cluster Galaxies (BCGs) residing in the centers of galaxy clusters are typically quenched giant ellipticals. A recent study hinted that star-forming galaxies with large disks, so-called superluminous spirals and lenticulars, are the BCGs of a ...
Andrade-Santos, Felipe +6 more
core +1 more source
LoCuSS: Testing hydrostatic equilibrium in galaxy clusters [PDF]
We test the assumption of hydrostatic equilibrium in an X-ray luminosity selected sample of 50 galaxy clusters at $0 ...
Graham P. Smith +23 more
semanticscholar +1 more source
Finding Galaxy Clusters using Voronoi Tessellations [PDF]
We present an objective and automated procedure for detecting clusters of galaxies in imaging galaxy surveys. Our Voronoi Galaxy Cluster Finder (VGCF) uses galaxy positions and magnitudes to find clusters and determine their main features: size, richness
Basilakos +32 more
core +3 more sources
Occurrence of radio halos in galaxy clusters - Insight from a mass-selected sample [PDF]
Giant radio halos (RH) are diffuse Mpc-scale synchrotron sources detected in a fraction of massive and merging galaxy clusters. An unbiased study of the statistical properties of RHs is crucial to constrain their origin and evolution.
V. Cuciti +8 more
semanticscholar +1 more source
Morphological Distribution of Galaxies in Some Nearby Clusters
We study the morphological distribution of galaxies in some nearby clusters, using the Sloan Digital Sky Survey – Data Release 9 (SDSS-DR9). The segregation between early-type galaxies and late-type ones is investigated in g – r / u – g color space ...
Rasheed Mariwan A., Mohammad Khalid K.
doaj +1 more source
On the origin of the intracluster light in massive galaxy clusters [PDF]
We present a pilot study on the origin and assembly history of the ICL for four galaxy clusters at 0.44 0.2 L* and that neither dwarf disruption nor major mergers with the BCG alone can explain the observed level of luminosity and remain consistent with ...
T. DeMaio +4 more
semanticscholar +1 more source
Galaxy Activity in Merging Binary Galaxy Clusters
We present the results of a study of galaxy activity in two merging binary clusters (A168 and A1750) using the Sloan Digital Sky Survey (SDSS) data supplemented with the data in the literature.
Adelman-McCarthy +84 more
core +1 more source
The Hydrangea simulations: galaxy formation in and around massive clusters [PDF]
We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in simulations of massive galaxy clusters (M200c = 1014–1015.4 M⊙) with baryon particle masses of ∼106 M⊙.
Y. Bah'e +14 more
semanticscholar +1 more source
Wide field imaging of distant clusters
Wide field imaging is key to understanding the build-up of distant clusters and their galaxy population. By focusing on the so far unexplored outskirts of clusters, where infalling galaxies first hit the cluster potential and the hot intracluster medium,
A. Diaferio, Tommaso Treu
core +2 more sources
Novel photo‐clickable triazine‐trione thermosets can be shaped and cured under mild conditions, including room and physiological temperatures. These materials are biocompatible and support osteogenic differentiation of bone marrow–derived mesenchymal stem cells on their surface.
Åshild Johansen +7 more
wiley +1 more source

