Results 141 to 150 of about 2,213,777 (304)
DIFFERENT APPROACHES FOR DARK MATTER HALOS OF CLUSTERS OF GALAXIES
To describe the density profile of dark matter halos of clusters of galaxies, we compare the approach based on the Schwarzschild-de Sitter metric with a recentlydeveloped mechanical one (discrete cosmology inside the cell of uniformity).
R. Brilenkov, M. Eingorn, A. Zhuk
doaj +1 more source
Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]
Botteon A+15 more
europepmc +1 more source
Galaxy Evolution in Clusters [PDF]
In this thesis, we aim to further elucidate the phenomenon of galaxy evolution in the environment of galaxy clusters using the methodology of numerical simulations. For that, we have developed hydrodynamic models in which idealized gas-rich galaxies move within the ICM of idealized galaxy clusters, allowing us to probe in a detailed and controlled ...
openaire +2 more sources
The ESO Distant Cluster Survey (EDisCS) is a photometric and spectroscopic study of the galaxy cluster population at two epochs, z~0.5 and z~0.8, drawn from the Las Campanas Distant Cluster Survey (LCDCS).
Anthony H. Gonzalez+7 more
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Strong suppression of heat conduction in a laboratory replica of galaxy-cluster turbulent plasmas. [PDF]
Meinecke J+34 more
europepmc +1 more source
Gravitational waves (GWs) from stellar binary black hole (sBBH) mergers can be strongly gravitational lensed by intervening galaxies/galaxy clusters. Only a few works have investigated cluster-lensed sBBH mergers by adopting oversimplified models, while ...
Zhiwei Chen+6 more
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Studying the Patterns of the Universe
The SDSS galaxy catalog is one of the best databases for galaxy distribution studies. The SDSS DR8 data is used to construct the galaxy cluster catalog.
Sepp T.+4 more
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Multipole analysis of cluster weak lensing shear in The Three Hundred project [PDF]
Weak gravitational lensing is an important tool to estimate the masses of galaxy clusters, as it allows us to directly access their projected surface mass density along the line of sight in a manner largely independent of their dynamical state. Moreover,
Payerne C.+4 more
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Search for clusters at high redshift - I. Candidate Lya emitters near 1138-262 at z=2.2 [PDF]
Radio, optical and X-ray observations of the powerful radio galaxy PKS 1138-262 at z=2.156 have suggested that this galaxy is a massive galaxy in the center of a forming cluster.
Carilli, C. L.+9 more
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Using a subsample of 79 nearby clusters from the RASS-SDSS galaxy cluster catalogue of Popesso et al. (2005a), we perform a regression analysis between the cluster integrated star formation rate (Sigma_SFR) the cluster total stellar mass (M_star), the ...
A. Biviano+5 more
core +3 more sources