Results 131 to 140 of about 1,030,336 (214)
A Large Mass of H_2 in the Brightest Cluster Galaxy in Zwicky 3146 [PDF]
We present the Spitzer/IRS mid-infrared spectrum of the infrared-luminous (L_(IR) = 4 × 10^(11) L_☉) brightest cluster galaxy (BCG) in the X-ray-luminous cluster Zwicky 3146 (Z3146; z = 0.29).
Fadda, D. +3 more
core
openIn questo progetto di tesi andrò a studiare la formazione e le proprietà fisiche delle galassie brillanti d'ammasso (in inglese brightest cluster galaxies, BCGs), esaminando in particolare i processi che regolano la formazione stellare all'interno ...
VOLPATO, SARA
core
We present a selection of candidates of clusters and protoclusters of galaxies identified in the photometric data of the HSC-SSP Wide Public Data Release 3 (PDR3), spanning the redshift range 0.1 ≤ z ≤ 2. The selection method, detailed in Vicentin et al.,
Marcelo C. Vicentin +4 more
doaj +1 more source
The Stellar Mass Function for Nine Massive Galaxy Clusters in the Local Universe
We measure galaxy stellar mass functions (SMFs) for nine of the most massive galaxy clusters in the local Universe (0.07
Jong-In Park +4 more
doaj +1 more source
JWST Photometry of Globular Cluster Populations in MACS0417.5−1154
Deep JWST imaging of the massive galaxy cluster MACS0417.5−1154, at redshift z = 0.443, reveals a huge population of globular clusters (GCs) and ultracompact dwarfs (UCDs) primarily distributed around its single central giant brightest cluster galaxy ...
William E. Harris +10 more
doaj +1 more source
Galaxy clusters enveloped by vast volumes of relativistic electrons. [PDF]
Cuciti V +14 more
europepmc +1 more source
Black hole mass estimates in brightest cluster galaxies
We present HST imaging and spectroscopic observations of three brightest cluster galaxies (BCGs), Abell 1836-BCG, Abell 2052-BCG, and Abell 3565-BCG, obtained with WFPC2, ACS, and STIS.
MIRALDA ESCUDÉ J. +13 more
core
Detection of Compton Scattering in the Jet of 3C 84
3C 84 is the brightest cluster galaxy in the Perseus Cluster. It is among the closest radio-loud active galaxies and among the very few that can be detected from low-frequency radio up to TeV γ -rays.
Ioannis Liodakis +79 more
doaj +1 more source
KINEMATICS OF 13 BRIGHTEST CLUSTER GALAXIES
Velocity dispersion profiles and rotation curves have been determined for a sample of 13 brightest duster galaxies (BCGs) in order to study their internal stellar kinematics and investigate their relationship to ellipticals.
ILLINGWORTH, G, FRANX, M, FISHER, D
core
Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]
Botteon A +15 more
europepmc +1 more source

