Results 51 to 60 of about 60,718 (195)
Galaxies in Clusters: the Observational Characteristics of Bow-Shocks, Wakes and Tails [PDF]
, 1999 The dynamical signatures of the interaction between galaxies in clusters and the intracluster medium (ICM) can potentially yield significant information about the structure and dynamical history of clusters.
Acreman, David M. +2 more
core +3 more sources
The Astrophysical Journal, 2023 We use the DR9 of the DESI legacy imaging survey and SDSS galaxy groups to measure the conditional luminosity function (CLF) for groups with halo mass M _h ≥ 10 ^12 M _⊙ and redshift 0.01 ≤ z ≤ 0.08, down to a limiting r -band magnitude of M _r = −10 to −
Jiacheng Meng +5 more
doaj +1 more source
The HI content of the Eridanus group of galaxies [PDF]
, 2004 The HI content of galaxies in the Eridanus group is studied using the GMRT observations and the HIPASS data. A significant HI deficiency up to a factor of 2-3 is observed in galaxies in the high galaxy density regions.
A. Biviano +31 more
core +3 more sources
The motions of clusters and group of galaxies
The Astrophysical Journal, 1994 25p plaintex submitted to The Astrophysical ...
Bahcall, Neta A. +2 more
openaire +3 more sources
A New X-ray Selected Sample of Very Extended Galaxy Groups from the ROSAT All-Sky Survey
, 2018 Some indications for tension have long been identified between cosmological constraints obtained from galaxy clusters and primary CMB measurements.
Erben, Thomas +4 more
core +1 more source
Gas-rich, Field Ultra-diffuse Galaxies Host Few Gobular Clusters
The Astrophysical Journal Letters, 2022 We present Hubble Space Telescope imaging of 14 gas-rich, low-surface-brightness galaxies in the field at distances of 25–36 Mpc, with mean effective radii and g -band central surface brightnesses of 1.9 kpc and 24.2 mag arcsec ^−2 .
Michael G. Jones +9 more
doaj +1 more source
X-ray bright groups and their galaxies [PDF]
, 2002 Combining X-ray data from the ROSAT PSPC and optical data drawn from the literature, we examine in detail the relationship between the X-ray and optical properties of X-ray bright galaxy groups. We find a relationship between optical luminosity and X-ray
Helsdon, Stephen F., Ponman, Trevor J.
core +3 more sources
Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
The Astrophysical JournalIt is yet to be understood how large-scale environments influence star formation activity in galaxy clusters. One recently proposed mechanism is that galaxy clusters can remain star forming when fed by infalling groups and star-forming galaxies from ...
Eunhee Ko +3 more
doaj +1 more source
Simulations of AGN Feedback in Galaxy Clusters and Groups [PDF]
AIP Conference Proceedings, 2009 4 pages, 2 figures, To appear in proceedings of the conference "The Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters", June 2009, Madison ...
Ewald Puchwein +4 more
openaire +3 more sources
The Blooming Tree Algorithm at Work: Clusters, Filaments, and Superclusters in the Field of A2029
The Astrophysical JournalThe Blooming Tree (BT) algorithm, based on the hierarchical clustering method, is designed to identify clusters, groups, and substructures from galaxy redshift surveys.
Heng Yu, Antonaldo Diaferio
doaj +1 more source