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brightest cluster galaxies

Exploring the progenitors of brightest cluster galaxies at z ∼ 2

Exploring the progenitors of brightest cluster galaxies at z ∼ 2

... of 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 ...

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Constraining cold accretion on to supermassive black holes: molecular gas in the cores of eight brightest cluster galaxies revealed by joint CO and CN absorption

Constraining cold accretion on to supermassive black holes: molecular gas in the cores of eight brightest cluster galaxies revealed by joint CO and CN absorption

... 18 brightest cluster galaxies lying in cool cores, from which we detect molecular gas in the core regions of eight via carbon monoxide (CO), cyanide (CN) and silicon monoxide (SiO) absorption ...

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The Link Between Extended Line Emission and AGN Feedback in Brightest Cluster Galaxies

The Link Between Extended Line Emission and AGN Feedback in Brightest Cluster Galaxies

... of brightest cluster ...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 ...

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Formation Pathways in Brightest Cluster Galaxies: Measuring the Distribution of Ages, Metallicities, and Hydrodynamics of Stellar Populations

Formation Pathways in Brightest Cluster Galaxies: Measuring the Distribution of Ages, Metallicities, and Hydrodynamics of Stellar Populations

... other galaxies will allow an inference into their ...23 brightest cluster galaxies as seen in Figure ...host cluster in order to separate the data into ...

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Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment

Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment

... nearby 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 ...

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The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs

The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs

... low-redshift 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 ...

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The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years

The evolution in the stellar mass of brightest cluster galaxies over the past 10 billion years

... the cluster, tidal stripping as a result of interactions with surrounding objects will ...the cluster to merge with the BCG, the amount of remaining stellar mass within the satellite available to be ...

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Stellar mass halo mass relation for the brightest central galaxies of X ray clusters since z~0 65

Stellar mass halo mass relation for the brightest central galaxies of X ray clusters since z~0 65

... the brightest cluster galaxies (BCGs) catalog for SPectroscoic IDentification of eROSITA Sources (SPIDERS) DR14 cluster program value-added ...

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The optical/X ray connection: intra cluster medium iron content and galaxy optical luminosity in 20 galaxy clusters

The optical/X ray connection: intra cluster medium iron content and galaxy optical luminosity in 20 galaxy clusters

... late-type galaxies, and of the brightest cluster galaxies ...from galaxies to the ICM, being very efficient for clusters in the temperature range 2 < kT (keV) < ...

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Brightest Cluster Galaxy Evolution Exploration: Comparing the Separation of Cluster X-ray Light and Visible Wavelength Galaxy Light with Spectral Data

Brightest Cluster Galaxy Evolution Exploration: Comparing the Separation of Cluster X-ray Light and Visible Wavelength Galaxy Light with Spectral Data

... Brightest Cluster Galaxies (BCGs), the brightest galaxy in a cluster of hundreds to thousands of galaxies, are some of the biggest, brightest, and most massive ...

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

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

... luminous cluster. Hydra-A is an archetype of a brightest cluster galaxy lying in a cooling flow; it has powerful radio jets and lobes emanating from its centre (Taylor et ...35 brightest ...

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The core flux of the brightest 10 μm galaxies in the southern sky

The core flux of the brightest 10 μm galaxies in the southern sky

... NGC 253. Figure A.1. This nearby starburst galaxy shows com- plex extended emission in all observed wavelengths: 8.6, 11.9 and 12.9 µ m. All images show two sources, the bright source seems to be resolved. The extended ...

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nIFTY galaxy cluster simulations – III  The similarity and diversity of galaxies and subhaloes

nIFTY galaxy cluster simulations – III The similarity and diversity of galaxies and subhaloes

... Section 3 shows that most codes reproduce the same bulk distribu- tion when running DM or NR simulations. The question is whether this agreement masks a variation in an individual object’s prop- erties. The properties of ...

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Using the Outskirts of Galaxy Clusters to Determine their Mass Accretion Rate

Using the Outskirts of Galaxy Clusters to Determine their Mass Accretion Rate

... the galaxies to estimate, through the escape velocity, the mass profile of the cluster at very large radii, up to several times the virial ...which galaxies are members of the cluster and ...

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Hubble’s Constant

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 ...

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No need for dark-matter, dark-energy or inflation, once ordinary matter is properly represented?

No need for dark-matter, dark-energy or inflation, once ordinary matter is properly represented?

... a cluster, if each galaxy in it were to vaporize, evenly distributing its mass across the entire cluster in a gaseous ...individual galaxies in the original solid cluster (recall the divergent ...

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The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies

The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies

... calibrated against the observed galaxy stellar mass function, the field galaxy size–mass relation and the BH mass–stellar mass relation at low redshift. Following this, the model then yields broad agree- ment with, among ...

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Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s

Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s

... a’ galaxies are a promising candidate for the intermediate stage of the transformation from star-forming spiral galaxies to passive ...the galaxies the last episode of star formation occurred in an ...

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The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field

The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field

... redshift galaxies, the existence of such objects, although unlikely, is still ...star-forming galaxies consistent with at most a small amount of dust ...

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A population of faint low surface brightness galaxies in the Perseus cluster core

A population of faint low surface brightness galaxies in the Perseus cluster core

... Perseus cluster core should be in process of tidal dis- ruption right now? – We do identify three LSB candidates in Perseus that show possible signs of disruption (see pan- els on the right hand side in ...the ...

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