Cluster galaxies
Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment
... brightest cluster galaxies (BCGs) from von der Linden et ...of galaxies with intermediate morphological classes (between ellipticals and cDs) suggests that the growth and morphological transformation ...
12
The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs
... brightest cluster galaxies (BCGs) and link their morphologies to their structural ...cD galaxies, ∼13 per cent are ellipticals, and ∼21 per cent be- long to the intermediate classes mostly between E ...
16
The formation history of massive cluster galaxies as revealed by CARLA
... Selecting galaxies within a constant 1 arcmin radius of the cluster centre at z < ...massive cluster galaxies, with the reddest colours, due to the SFR–density ...massive cluster ...
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The Link Between Extended Line Emission and AGN Feedback in Brightest Cluster Galaxies
... These galaxies are central to the cycles of galaxy feedback that are thought to occur in the cores of massive galaxy ...central galaxies is the leading candidate to moderate the level of gas cooling that ...
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Exploring the progenitors of brightest cluster galaxies at z ∼ 2
... brightest cluster galaxies (BCGs) from z ∼ 2 to z ∼ ...late-type galaxies, exhibiting less concentrated profiles than their early- type local ...other galaxies of similar mass at the same ...
22
The KMOS Cluster Survey (KCS) III Fundamental Plane of Cluster Galaxies at z ≃ 1 80 in JKCS 041
... Some areas of the spectra were affected by strong sky line residuals even after reduction. The three worst af- fected bands, when shifted to the rest frame (assum- ing z = 1.80), corresponded roughly to ∼ 3570–3750, ...
24
GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024 0+1652 at z=0 395
... galaxy cluster ZwCl 0024 + 1652 (here- after referred to as Cl0024) at z = ...star-forming galaxies and AGNs is ...of galaxies by means of emission (rather than absorp- tion) ...
22
Chemical evolution of star-forming galaxies in the overdense environment
... infalling galaxies is proportional to the density of the ICM at the location of the galaxy and the square of its infall ...of cluster galaxies ...field galaxies has a spatial extent almost two ...
146
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
... realistic galaxies is more than an or- der of magnitude higher than that in most previous cluster ...of cluster galaxies, the interaction of galaxies with the ICM, the formation of ...
19
MC2: A Deeper Look at ZwCl 2341.1+0000 with Bayesian Galaxy Clustering and Weak Lensing Analyses
... We used the previously discussed number density and luminosity maps, as well as similar maps made from the spectroscopic catalog and a convergence map made in our weak lensing analysis (this will be discussed later), to ...
63
Iannuzzi, Francesca (2012): Simulating structure formation with high precision: numerical techniques, dynamics and the evolution of substructures. Dissertation, LMU München: Fakultät für Physik
... the cluster environment has major consequences on the evolution of the internal properties of the ...satellite galaxies moving within a cluster ...star-forming, cluster galaxies as ...
158
Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s
... 13 galaxies with disc mor- phologies and strong H δ absorption in the cluster AC114 (also known as Abell S1077; Abell, Corwin & Olowin 1989) at z ∼ ...star-forming galaxies by Couch & ...
13
Ultra red Galaxies Signpost Candidate Protoclusters at High Redshift
... densities of (physically associated) DSFGs (i.e. a ‘proto- cluster’ — Muldrew et al. 2015; Casey 2016). Such sys- tems have already been discovered in the z > 3 Universe via their submillimeter (submm) ...
24
A mature galaxy cluster at z= 1 58 around the radio galaxy 7C 1753+6311
... of galaxies in the densest environments, clusters, it is important to study their progenitors: high-redshift protocluster ...massive cluster cores at z ...
8
The XXL Survey: XXXIV. Double irony in XXL-North. A tale of two radio galaxies in a supercluster at z = 0.14
... the galaxies with a spec- troscopic redshift from the GAMA database between ...eight cluster members, five of which are securely detected clusters in X-rays (C1 ...The cluster hosting the Exemplar, ...
23
H ATLAS: a candidate high redshift cluster/protocluster of star forming galaxies
... and the lack of a bright optical or radio counterpart (see eg. Negrello et al. 2010 for a discussion of the selection of lens candidates in H-ATLAS and other Herschel surveys). This source was therefore observed ...
16
Globular Cluster Populations: First Results from S4G Early-type Galaxies
... Globular cluster candidates at these distances, in images of this angular resolution, will appear as point ...stars, galaxies of small angular size, and globular ...not cluster about the ...globular ...
19
The ESO nearby Abell cluster survey. IV. The fundamental plane of clusters of galaxies
... We have confirmed the result of Schaeffer et al. (1993) that clusters of galaxies populate a Fundamental Plane (FP). The orientation of the FP of clusters can be determined reasonably well from our ENACS data, but ...
13
Low metallicities and old ages for three ultra diffuse galaxies in the Coma cluster
... three galaxies must have been truncated at high ...other galaxies from the ...Coma cluster obtained as part of the Deep Coma program ( ...type galaxies from stacked SDSS spectra by Conroy et ...
13
Hubble’s Constant
... any cluster of galaxies, as the Virgo cluster, which is the nearest rich cluster of galaxies, and use one of the galaxies as a measured unit in order to obtain the distances of ...
5