Results 21 to 30 of about 14,082 (274)
Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies [PDF]
The Astrophysical Journal, 2018 We present a study of 107 galaxies, groups, and clusters spanning ∼3 orders of magnitude in mass, ∼5 orders of magnitude in central galaxy star formation rate (SFR), ∼4 orders of magnitude in the classical cooling rate ( ) of the intracluster medium (ICM)
M. McDonald +3 more
semanticscholar +6 more sources
Diffuse Baryons in Groups and Clusters of Galaxies [PDF]
The Astrophysical Journal, 1998 To predict the X-ray observables associated to the diffuse baryons in clusters of galaxies, we develop a new physical approach to model such a hot intra-cluster plasma. Such approach is based on punctuated equilibria. and comprises the following blocks: Monte Carlo ``merging histories'' of dark matter potential wells; the central hydrostatic ...
A. Cavaliere, N. Menci, P. Tozzi
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Dark Matter in Groups and Clusters of Galaxies [PDF]
International Astronomical Union Colloquium, 2000 AbstractWe compare the characteristics of stellar populations with those of dark halos. Dark matter around galaxies, and in groups, clusters and voids is discussed. Modern data suggest that the overall density of matter in the Universe is ΩM = 0.3 ± 0.1, about 80 % of this matter is nonbaryonic dark matter, and about 20 % is baryonic, mostly in the ...
J. Einasto, M. Einasto
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The colours of satellite galaxies in groups and clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2008 Current models of galaxy formation predict satellite galaxies in groups and clusters that are redder than observed. We investigate the effect on the colours of satellite galaxies produced by the ram pressure stripping of their hot gaseous atmospheres as the satellites orbit within their parent halo. We incorporate a model of the stripping process based
Andreea S. Font +8 more
openalex +7 more sources
Accretion of galaxy groups into galaxy clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We study the role of group infall in the assembly and dynamics of galaxy clusters in ΛCDM. We select 10 clusters with virial mass M200 ∼ 1014 $\rm M_\odot$ from the cosmological hydrodynamical simulation Illustris and follow their galaxies with stellar mass M⋆ ≥ 1.5 × 108 $\rm M_\odot$.
Laura V. Sales +3 more
openaire +4 more sources
INDIVIDUAL AND GROUP GALAXIES IN CNOC1 CLUSTERS [PDF]
The Astrophysical Journal, 2009 ApJ ...
I. H. Li, H. K. C. Yee, E. Ellingson
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Properties of Fossil Groups of Galaxies
Universe, 2021 We review the formation and evolution of fossil groups and clusters from both the theoretical and the observational points of view. In the optical band, these systems are dominated by the light of the central galaxy.
J. Alfonso L. Aguerri, Stefano Zarattini
doaj +1 more source
The Effect of Splashback on Weak Lensing Mass Estimates of Galaxy Clusters and Groups
The Open Journal of Astrophysics, 2023 The splashback radius of a dark matter halo, which corresponds to the first apocenter radius reached by infalling matter and substructures, has been detected around galaxy clusters using a multitude of observational methods, including weak lensing ...
Yuanyuan Zhang +5 more
doaj +2 more sources
Galaxy and mass assembly (GAMA): the clustering of galaxy groups [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT 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 autocorrelation function, we instead measure the ...
S D Riggs +6 more
openaire +4 more sources