Results 21 to 30 of about 1,040 (235)

Parsec-scale properties of brightest cluster galaxies [PDF]

open access: yesAstronomy and Astrophysics, 2010
20 pages, 10 figures, accepted for publication in A& ...
LIUZZO, ELISABETTA   +3 more
openaire   +3 more sources

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

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 CLUSTERS AT HIGH REDSHIFT AND EVOLUTION OF BRIGHTEST CLUSTER GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2011
10 pages, 14 figures, 2 tables; added reference, corrected typos; Table 2 is available at http://zmtt.bao.ac.cn/wzl/CV_wen ...
Wen, Z. L., Han, J. L.
openaire   +2 more sources

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

How special are brightest group and cluster galaxies? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
Abstract We use the Sloan Digital Sky Survey (SDSS) to construct a sample of 625 brightest group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in stellar mass, redshift and colour. We investigate how the systematic properties of BCGs depend on stellar mass and on their privileged location near the cluster ...
von der Linden, Anja   +3 more
openaire   +4 more sources

Alignment of brightest cluster galaxies with their host clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2010
15 pages, 12 Figures, 10 Tables, Accepted for publication in ...
Niederste-Ostholt, Martin   +4 more
openaire   +3 more sources

The Brightest UV-selected Galaxies in Protoclusters at z ∼ 4: Ancestors of Brightest Cluster Galaxies? [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract We present the results of a survey of the brightest UV-selected galaxies in protoclusters. These proto-brightest cluster galaxy (proto-BCG) candidates are drawn from 179 overdense regions of g-dropout galaxies at z ∼ 4 from the Hyper Suprime-Cam Subaru Strategic Program identified previously as good protocluster candidates. This
Kei Ito   +15 more
openaire   +5 more sources

Ionized nebulae surrounding brightest cluster galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
We present IFU observations of six emission-line nebulae that surround the central galaxy of cool core clusters. Qualitatively similar nebulae are observed in cool core clusters even when the dynamics and possibly formation and excitation source are different.
N. A. Hatch   +2 more
openaire   +3 more sources

Precision Modeling of JWST's First Cluster Lens SMACS J0723.3–7327

open access: yesThe Astrophysical Journal, 2023
Exploiting the fundamentally achromatic nature of gravitational lensing, we present a lens model for the massive galaxy cluster SMACS J0723.3−7323 (SMACS J0723; z = 0.388) that significantly improves upon earlier work.
Guillaume Mahler   +14 more
doaj   +1 more source

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