An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic web. As galaxies are accreted they are affected by their local environment before they enter (pre-processing), and traverse the cluster potential.
Ulrike Kuchner +8 more
openaire +4 more sources
Evidence for AGN Feedback in Galaxy Clusters and Groups
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
doaj +1 more source
ФОРМЫ ТРЕХКОМПОНЕНТНЫХ СВЕРХСКОПЛЕНИЙ ГАЛАКТИК
Odessa Astronomical Publications, 2011 We analyzed the shapes of galaxy superclusters, contains only 3 galaxy clusters. The superclusters were found using PF Catalogue Galaxy Clusters and Groups covering 5000 square degrees as input data.
Е. А. Панько
doaj +1 more source
The similarity of the stellar mass fractions of galaxy groups and clusters [PDF]
, 2013 We employ a large sample of 20171 optically-selected groups and clusters at 0.15 < z < 0.4 in the SDSS to investigate how the stacked stellar mass fraction varies across a wide range of total mass, $M_{500}$.
J. M. Budzynski +3 more
semanticscholar +1 more source
A Census of Baryons in Galaxy Clusters and Groups [PDF]
, 2007 We determine the contribution of stars in galaxies, intracluster stars, and the intracluster medium to the total baryon budget in nearby galaxy clusters and groups. We find that the baryon mass fraction (f_b) within r500 is constant for systems with M500
Gonzalez, Anthony H. +2 more
core +1 more source
Galaxy evolution in groups and clusters: star formation rates, red sequence fractions and the persistent bimodality [PDF]
, 2011 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 ...
A. Wetzel, J. Tinker, C. Conroy
semanticscholar +1 more source
Exploring diffuse radio emission in galaxy clusters and groups with uGMRT and SKA [PDF]
Journal of astrophysics and astronomy, 2022 Diffuse radio emission has been detected in a considerable number of galaxy clusters and groups, revealing the presence of pervasive cosmic magnetic fields, and of relativistic particles in the large scale structure of the Universe.
S. Paul +15 more
semanticscholar +1 more source
AEGIS: Chandra Observation of DEEP2 Galaxy Groups and Clusters [PDF]
, 2006 We present a 200 ksec Chandra observation of seven spectroscopically selected, high redshift (0.75 < z < 1.03) galaxy groups and clusters discovered by the DEEP2 Galaxy Redshift Survey in the Extended Groth Strip (EGS). X-ray emission at the locations of
Alison L. Coil +13 more
core +2 more sources
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. Willis +16 more
semanticscholar +1 more source
Galaxy and cluster biasing from Local Group dynamics [PDF]
Monthly Notices of the Royal Astronomical Society, 2000 Comparing the gravitational acceleration induced on the Local Group of galaxies by different tracers of the underline density field we estimate, within the linear gravitational instability theory and the linear biasing ansatz, their relative bias factors. Using optical SSRS2 galaxies, IRAS (PSCz) galaxies and Abell/ACO clusters, we find b_{O,I} ~ 1.21 +
Plionis, M. +6 more
openaire +3 more sources