The radial structure of galaxy groups and clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2003 Simple self-consistent models of galaxy groups and clusters are tested against the re-sults of high-resolutionadiabatic gasdynamicalsimulations.
Y. Ascasíbar +3 more
semanticscholar +7 more sources
The cosmological constant derived via galaxy groups and clusters [PDF]
European Physical Journal C: Particles and Fields, 2019 The common nature of dark matter and dark energy is argued in Gurzadyan (Eur Phys J Plus 134:14, 2019) based on the approach that the cosmological constant $$\varLambda $$ Λ enters the weak-field General Relativity following from Newton theorem on the ...
V. G. Gurzadyan, A. Stepanian
doaj +2 more sources
Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing [PDF]
, 2006 We present results of a measurement of the shape of the density profile of galaxy groups and clusters traced by 43 335 Luminous Red Galaxies (LRGs) with spectroscopic redshifts from the Sloan Digital Sky Survey (SDSS). The galaxies are selected such that
Rachel Mandelbaum +5 more
openalex +3 more sources
Kinematics of the diffuse intragroup and intracluster light in groups and clusters of galaxies in the local universe within 100 Mpc distance [PDF]
Frontiers in Astronomy and Space Sciences, 2022 Nearly all intragroup (IGL) and intracluster light (ICL) comes from stars that are not bound to any single galaxy but were formed in galaxies and later unbound from them.
Magda Arnaboldi, Ortwin Gerhard
doaj +2 more sources
Erratum: The XMM Large-Scale Structure survey: an initial sample of galaxy groups and clusters to a redshift z < 0.6 [PDF]
, 2005 We present X-ray and optical spectroscopic observations of 12 galaxy groups and clusters identified within the X-ray Multi-Mirror (XMM) Large-Scale Structure (LSS) survey.
J. P. Willis +16 more
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Dust accretion and destruction in galaxy groups and clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 We examine the dust distribution around a sample of 70000 low-redshift galaxy groups and clusters derived from the Sloan Digital Sky Survey (SDSS). By correlating spectroscopically identified background quasars with the galaxy groups, we obtain the ...
S. McGee, M. Balogh
semanticscholar +5 more sources
Evidence for AGN Feedback in Galaxy Clusters and Groups [PDF]
Advances in Astronomy, 2012 The current generation of flagship X-ray missions, Chandra and XMM-Newton, has changed our understanding of the so-called “cool-core” galaxy clusters and groups.
Myriam Gitti +2 more
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Implications of the remarkable homogeneity of galaxy groups and clusters [PDF]
, 2010 We measure the diversity of galaxy groups and clusters with mass M > 1013 h−1 M⊙, in terms of the star formation history of their galaxy populations, for the purpose of constraining the mass scale at which environmentally important processes play a role ...
Michael L. Balogh, Sean McGee
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Galaxy evolution in groups and clusters: star formation rates, red sequence fractions and the persistent bimodality [PDF]
, 2012 Using galaxy group/cluster catalogues created from the Sloan Digital Sky Survey Data Release 7, we examine in detail the specific star formation rate (SSFR) distribution of satellite galaxies and its dependence on stellar mass, host halo mass and halo ...
Andrew Wetzel +2 more
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Ram pressure profiles in galaxy groups and clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2011 Using a hybrid method that combines non-radiative hydrodynamical simulations with a semi-analytic model of galaxy formation, we determine the ram pressure experienced by galaxies in haloes with virial masses 12.5 ≤ log (M200/ h-1 M⊙) < 15.35 as a ...
T. Tecce, S. Cora, P. Tissera
semanticscholar +7 more sources