Results 21 to 30 of about 336 (182)
Are Brightest Cluster Galaxies Special?
Abstract A longstanding question when studying Brightest Cluster Galaxies (BCGs) and their evolution is whether their luminosities are statistical extremes of the luminosity distribution of other cluster member galaxies, or whether their luminosities follow a different,“special” distribution.
Savannah Pobre +3 more
openaire +1 more source
Cluster Selection and the Evolution of Brightest Cluster Galaxies
Accepted for publication in ApJL. 4 pages including 4 figures, uses emulateapj.sty (included)
Burke, D. J. +2 more
openaire +3 more sources
The Brightest UV-selected Galaxies in Protoclusters at z ∼ 4: Ancestors of Brightest Cluster Galaxies? [PDF]
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
The Evolution of AGN Activity in Brightest Cluster Galaxies
Abstract We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg2 South Pole Telescope (SPT)-Sunyaev–Zel’dovich cluster sample. We describe a process for identifying active galactic nuclei (AGN) in brightest cluster galaxies (BCGs) based on WISE mid-IR color and redshift ...
Taweewat Somboonpanyakul +81 more
openaire +11 more sources
THE DYNAMICAL STATE OF BRIGHTEST CLUSTER GALAXIES AND THE FORMATION OF CLUSTERS [PDF]
114 pages, 9 figures, full version of tables 1 and 2; accepted to appear in ...
Coziol, R. +4 more
openaire +2 more sources
A detection of wobbling brightest cluster galaxies within massive galaxy clusters [PDF]
A striking signal of dark matter beyond the standard model is the existence of cores in the centre of galaxy clusters. Recent simulations predict that a Brightest Cluster Galaxy (BCG) inside a cored galaxy cluster will exhibit residual wobbling due to previous major mergers, long after the relaxation of the overall cluster.
Harvey, David +3 more
openaire +3 more sources
MAJOR CLUSTER MERGERS AND THE LOCATION OF THE BRIGHTEST CLUSTER GALAXY [PDF]
Using a large N-body cosmological simulation combined with a subgrid treatment of galaxy formation, we study the formation and evolution of the galaxy and cluster population in a comoving volume (100 Mpc)^3 in a LCDM universe. At z = 0, our computational volume contains 1788 clusters with mass M_cl > 1.1x10^12 Msun, including 18 massive clusters ...
Hugo Martel +2 more
openaire +2 more sources
Environmental dependence of the structure of brightest cluster galaxies [PDF]
11 pages, accepted for publication in ...
Brough, Sarah +4 more
openaire +3 more sources
Models for the magnitude-distribution of brightest cluster galaxies [PDF]
Abstract submitted to AAS.
Bernstein, J. P., Bhavsar, Suketu P.
openaire +2 more sources
The shapes of brightest cluster galaxies
The mean isophotal axis ratios are computed for a complete sample of 119 brightest cluster galaxies (BCGs) in Abell clusters. The cumulative distribution function F(q) of axis ratios for the BCGs differs from F(q) for a sample of ordinary elliptical galaxies at only the P=0.14 probability level, as measured by a Kolmogorov Smirnov test.
Barbara S. Ryden +2 more
openaire +1 more source

