Results 41 to 50 of about 89,392 (297)

The Angular Momentum of Brightest Cluster Galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2012
AbstractMassive Brightest Cluster Galaxies (BCGs) are observed to have a range of angular momenta, suggesting a variety of merging histories.
Brough, S, Tran, K-V, von der Linden, A
openaire   +3 more sources

The XMM Cluster Survey: The Stellar Mass Assembly of Fossil Galaxies [PDF]

open access: yes, 2012
This paper presents both the result of a search for fossil systems (FSs) within the XMM Cluster Survey and the Sloan Digital Sky Survey and the results of a study of the stellar mass assembly and stellar populations of their fossil galaxies. In total, 17
A. Kathy Romer   +60 more
core   +2 more sources

The different growth pathways of Brightest Cluster Galaxies and the Intra-Cluster Light [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We study the growth pathways of brightest central galaxies (BCGs) and intracluster light (ICE) by means of a semi-analytic model. We assume that ICL forms by stellar stripping of satellite galaxies and violent processes during mergers, and implement two ...
E. Contini, S. K. Yi, X. Kang
semanticscholar   +1 more source

LINEAR SUBSTRUCTURES IN GALAXY CLUSTERS

open access: yesOdessa Astronomical Publications, 2019
We propose detailed scheme that is describing the morphology of linear substructures in galaxy clusters. Our base morphological scheme di- vides galaxy clusters using numerical criteria according the parameters: concentration to the cluster center, the ...
E. Panko   +3 more
doaj   +1 more source

Parsec Scale Properties of Brightest Cluster Galaxies. [PDF]

open access: yesProceedings of The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting — PoS(IX EVN Symposium), 2009
6 pages, 2 figures. Contributed talk. To be published in the proceedings of "The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting", September 23-26, 2008, Bologna ...
Giovannini, G.   +2 more
openaire   +3 more sources

Galaxy Orientations in the Coma Cluster [PDF]

open access: yes, 2007
We have examined the orientations of early-type galaxies in the Coma cluster to see whether the well-established tendency for brightest cluster galaxies to share the same major axis orientation as their host cluster also extends to the rest of the galaxy
Binggeli B.   +6 more
core   +2 more sources

The ROSAT Brightest Cluster Sample — III. Optical spectra of the central cluster galaxies [PDF]

open access: yes, 1999
We present new spectra of dominant galaxies in X-ray selected clusters of galaxies, which combine with our previously published spectra to form a sample of 256 dominant galaxies in 215 clusters.
C. Crawford   +9 more
semanticscholar   +1 more source

The Galaxy Population of Cluster RXJ0848+4453 at z=1.27 [PDF]

open access: yes, 2001
We present a study of the galaxy population in the cluster RXJ0848+4453 at z=1.27, using deep HST NICMOS and WFPC2 images. We morphologically classify all galaxies to K_s=20.6 that are covered by the HST imaging, and determine photometric redshifts using
Andreon S.   +11 more
core   +2 more sources

THE ELLIPTICITIES OF GALAXIES IN GALAXY CLUSTERS OF DIFFERENT MORPHOLOGICAL TYPE

open access: yesOdessa Astronomical Publications, 2014
The distribution of galaxy ellipticities was analyzed for 207 rich PF galaxy clusters found in the Munster Red Sky Survey Galaxy Catalogue. Clusters with BM types from a comparison with the ACO catalogue were also classified on the new scheme.
E. A. Panko, P. Flin
doaj   +1 more source

Brightest Cluster Galaxy Alignments in Merging Clusters [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract The orientations of brightest cluster galaxies (BCGs) and their host clusters tend to be aligned, but the mechanism driving this is not clear. To probe the role of cluster mergers in this process, we quantify alignments of 38 BCGs in 22 clusters undergoing major mergers (up to ∼1 Gyr after first pericenter).
David Wittman   +2 more
openaire   +4 more sources

Home - About - Disclaimer - Privacy