Results 21 to 30 of about 6,069 (215)
ON THE BARYON FRACTIONS IN CLUSTERS AND GROUPS OF GALAXIES [PDF]
We present the baryon fractions of 2MASS groups and clusters as a function of cluster richness using total and gas masses measured from stacked ROSAT X-ray data and stellar masses estimated from the infrared galaxy catalogs. We detect X-ray emission even in the outskirts of clusters, beyond r_200 for richness classes with X-ray temperatures above 1 keV.
Dai, Xinyu +3 more
openaire +2 more sources
Scaling Properties of Galaxy Groups
Galaxy groups and poor clusters are more common than rich clusters, and host the largest fraction of matter content in the Universe. Hence, their studies are key to understand the gravitational and thermal evolution of the bulk of the cosmic matter ...
Lorenzo Lovisari +3 more
doaj +1 more source
INDIVIDUAL AND GROUP GALAXIES IN CNOC1 CLUSTERS [PDF]
ApJ ...
Li, I. H., Yee, H. K. C., Ellingson, E.
openaire +3 more sources
The 2dF Galaxy Redshift Survey: the clustering of galaxy groups [PDF]
16 pages.
Padilla, Nelson D. +29 more
openaire +8 more sources
The cosmological constant derived via galaxy groups and clusters
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 +1 more source
The motions of clusters and group of galaxies
25p plaintex submitted to The Astrophysical ...
Bahcall, Neta A. +2 more
openaire +3 more sources
THE GALAXY CONTENT OF SDSS CLUSTERS AND GROUPS [PDF]
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. We investigate the dependence of Brightest Cluster Galaxy (BCG) luminosity, and the distributions of satellite galaxy luminosity and satellite color, on cluster properties over the redshift range ...
Hansen, Sarah M. +3 more
openaire +2 more sources
Not all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low surface brightness component of groups/clusters generally found
Emanuele Contini
doaj +1 more source
Globular Clusters around Galaxies in Groups [PDF]
We have obtained deep photometry of NGC 1199 (in HCG 22) and NGC 6868 (in the Telescopium group). Both galaxies are the optically brightest galaxies of their groups. Our analysis of B and R images taken with the Keck II and the VLT/ESO telescopes, detected a population of globular clusters around both galaxies, with total specific frequencies SN = 1.7 ±
Da Rocha, Martine +4 more
openaire +7 more sources
THE PECULIARITIES IN O-TYPE GALAXY CLUSTERS
We present the results of analysis of 2D distribution of galaxies in galaxy cluster fields. The Catalogue of Galaxy Clusters and Groups PF (Panko & Flin) was used as input observational data set.
E. A. Panko, S. I. Emelyanov
doaj +1 more source

