Results 121 to 130 of about 1,030,336 (214)

Witnessing the Formation of a Brightest Cluster Galaxy in a Nearby X-Ray Cluster

open access: yes, 2010
The central dominant galaxies in galaxy clusters constitute the most massive and luminous galaxies in the universe. Despite this, the formation of these brightest cluster galaxies (BCGs) and the impact of this on the surrounding cluster environment ...
Lei Bai   +11 more
core   +1 more source

The Journey to Dominance: How Brightest Cluster Galaxies Evolve Differently from Other Massive Galaxies

open access: yesThe Astrophysical Journal
We use the L-GALAXIES semianalytic model to investigate the evolution of brightest cluster galaxies (BCGs) found in clusters at z  ∼ 0. BCGs are typically located in the central region of galaxy clusters, near the bottom of the potential well, exposing ...
Marcelo C. Vicentin   +5 more
doaj   +1 more source

XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029

open access: yesThe Astrophysical Journal Letters
We present XRISM Resolve observations of the core of the hot, relaxed galaxy cluster Abell 2029 (A2029). We find that the line-of-sight bulk velocity of the intracluster medium (ICM) within the central 180 kpc is at rest with respect to the brightest ...
XRISM Collaboration   +138 more
doaj   +1 more source

Evolution of the Brightest Cluster Galaxies [PDF]

open access: yes, 2016
In this thesis, I explore the evolution of the brightest cluster galaxies (BCGs) over the last 10 billion years through detailed studies of both local BCGs from SDSS and their high-z progenitors from CANDELS UDS.\ud \ud First, I study a large sample of local BCGs and link their morphologies to their structural properties.
openaire   +1 more source

Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium

open access: yesThe Astrophysical Journal
We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM).
Arsen Levitskiy   +4 more
doaj   +1 more source

Feedback and brightest cluster galaxy formation: ACS observations of the radio galaxy TNJ J1338-1942 AT z=4.1

open access: yes, 2005
We present deep optical imaging of the z 4: 1 radio galaxy TN J1338 - 1942, obtained using the Advanced Camera for Surveys ( ACS) on board the Hubble Space Telescope, as well as ground- based near- infrared imaging data from the European Southern ...
Infante L   +45 more
core   +1 more source

Environmental Imprints on the Assembly of the Cool Gas around Bright Cluster Galaxies

open access: yesThe Astrophysical Journal Letters
Galaxy clusters represent extreme cosmic laboratories where environmental processes dramatically reshape their constituent galaxies, yet their effect on the gaseous halos of central galaxies remains poorly constrained.
Runyu Zhu   +16 more
doaj   +1 more source

Weak-lensing Characterization of the Dark Matter in 29 Merging Clusters that Exhibit Radio Relics

open access: yesThe Astrophysical Journal Supplement Series
We present a multiwavelength analysis of 29 merging galaxy clusters that exhibit radio relics. For each merging system, we perform a weak-lensing analysis on Subaru optical imaging.
Kyle Finner   +7 more
doaj   +1 more source

Warm and Cold Molecular Gas in the Cluster Center of MACS 1931−26 with JWST and ALMA

open access: yesThe Astrophysical Journal
We perform one of the first spatially resolved studies of warm (>100 K) and cold (10–100 K) molecular gas in the circumgalactic medium (CGM), focusing on the brightest cluster galaxy (BCG) of a cool-core galaxy cluster, MACS 1931−26, at z = 0.35.
L. Ghodsi   +11 more
doaj   +1 more source

A distinct radial acceleration relation across the brightest cluster galaxies and galaxy clusters

open access: yesAstronomy & Astrophysics
Recent studies reveal a radial acceleration relation (RAR) in galaxies, which illustrates a tight empirical correlation connecting the observational acceleration and the baryonic acceleration with a characteristic acceleration scale. However, a distinct RAR has been revealed on brightest cluster galaxy (BCG) cluster scales with a seventeen-times-larger
Yong Tian   +4 more
openaire   +2 more sources

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