Results 1 to 10 of about 59,561 (180)

The Formation of the Brightest Cluster Galaxy and Intracluster Light in Cosmological N-body Simulations with the Galaxy Replacement Technique [PDF]

open access: yesThe Astrophysical Journal, 2023
We investigate the formation channels of the intracluster light (ICL) and the brightest cluster galaxy (BCG) in clusters at z = 0. For this, we perform multi-resolution cosmological N -body simulations using the “galaxy replacement technique.” We study ...
Kyungwon Chun   +4 more
doaj   +2 more sources

Brightest Cluster Galaxy Alignments in Merging Clusters [PDF]

open access: yesThe Astrophysical Journal, 2018
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 ...
D. Wittman, Drake Foote, N. Golovich
semanticscholar   +6 more sources

Are Brightest Cluster Galaxies Special?

open access: yesResearch Notes of the AAS, 2023
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 ...
Savannah Pobre   +3 more
semanticscholar   +2 more sources

A detection of wobbling brightest cluster galaxies within massive galaxy clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
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 ...
D. Harvey   +3 more
semanticscholar   +5 more sources

Brightest Cluster Galaxy Profile Shapes [PDF]

open access: yesThe Astrophysical Journal, 1996
We model the surface brightness profiles of a sample of 119 Abell Brightest Cluster Galaxies (BCG), finding a generalised deVaucouleurs R^{1/n} law, where n is a free parameter, to be appropriate.
A. Graham, T. Lauer, M. Postman
semanticscholar   +4 more sources

Structure of Brightest Cluster Galaxies and Intracluster Light [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2019
Observations of 170 local (z ≲ 0.08) galaxy clusters in the northern hemisphere have been obtained with the Wendelstein Telescope Wide Field Imager (WWFI).
M. Kluge   +8 more
semanticscholar   +5 more sources

Intrinsic Shapes of Brightest Cluster Galaxies

open access: yesThe Astrophysical Journal, 2022
Abstract We discuss the statistical distribution of galaxy shapes and viewing angles under the assumption of triaxiality by deprojecting observed surface brightness profiles of 56 brightest cluster galaxies (BCGs) coming from a recently published large deep-photometry sample.
Stefano de Nicola   +7 more
openaire   +3 more sources

Chandra Observations of Abell 2261 Brightest Cluster Galaxy, a Candidate Host to a Recoiling Black Hole [PDF]

open access: yes, 2020
We use Chandra X-ray observations to look for evidence of a recoiling black hole from the brightest cluster galaxy in Abell 2261 (A2261-BCG). A2261-BCG is a strong candidate for a recoiling black hole because of its large, flat stellar core, revealed by ...
K. Gültekin   +6 more
semanticscholar   +1 more source

Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
Active galactic nuclei play a crucial role in the accretion and ejection of gas in galaxies. Although their outflows are well studied, finding direct evidence of accretion has proved very difficult and has so far been done for very few sources.
T. Rose   +40 more
semanticscholar   +1 more source

The Dust and Molecular Gas in the Brightest Cluster Galaxy in MACS 1931.8-2635 [PDF]

open access: yesAstrophysical Journal, 2019
We present new Atacama Large Millimeter Array observations of the molecular gas and far-infrared continuum around the brightest cluster galaxy (BCG) in the cool-core cluster MACS 1931.8-2635. Our observations reveal (1.9 ± 0.3) × 1010 M⊙ of molecular gas,
K. Fogarty   +8 more
semanticscholar   +1 more source

Home - About - Disclaimer - Privacy