Results 1 to 10 of about 2,651,791 (306)
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 +10 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 +4 more sources
THE GALAXY CONTENT OF SDSS CLUSTERS AND GROUPS [PDF]
The Astrophysical Journal, 2009 Imaging data from the Sloan Digital Sky Survey are used to characterize the population of galaxies in groups and clusters detected with the MaxBCG algorithm.
Sarah M. Hansen +3 more
core +10 more sources
Individual and Group Galaxies in CNOC1 clusters [PDF]
Astrophys.J.698:83-98,2009, 2009 Using wide-field $BVR_cI$ imaging for a sample of 16 intermediate redshift ($0.17 < z < 0.55$) galaxy clusters from the Canadian Network for Observational Cosmology (CNOC1) Survey, we investigate the dependence of cluster galaxy populations and their evolution on environment.
I. H. Li, H. K. C. Yee, E. Ellingson
arxiv +7 more sources
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 +8 more sources
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 +11 more sources
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
semanticscholar +6 more sources
Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 We explore the clustering of galaxy groups in the Galaxy and Mass Assembly (GAMA) survey to investigate the dependence of group bias and profile on separation scale and group mass. Due to the inherent uncertainty in estimating the group selection function, and hence the group auto-correlation function, we instead measure the projected galaxy--group ...
S D Riggs +6 more
arxiv +6 more sources
Galaxy clusters and groups in the ALHAMBRA Survey [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 We present a catalogue of 348 galaxy clusters and groups with $0 ...
Aguerri, J. Alfonso L. +37 more
core +12 more sources
Integrated HI emission in galaxy groups and clusters [PDF]
, 2017 The integrated HI emission from hierarchical structures such as groups and clusters of galaxies can be detected by FAST at intermediate redshifts. Here we propose to use FAST to study the evolution of the global HI content of clusters and groups over ...
M. Ai, M. Zhu, Jian Fu
semanticscholar +3 more sources