Results 31 to 40 of about 188 (137)
G0.253+0.016: A CENTRALLY CONDENSED, HIGH-MASS PROTOCLUSTER [PDF]
57 pages. 29 figures.
J. M. Rathborne +11 more
openaire +6 more sources
The most luminous quasars at z > 6 are suspected to be both highly clustered and to reside in the most massive dark matter halos in the early universe, making them prime targets to search for galaxy overdensities and/or protoclusters. We search for Lyman-
Jaclyn B. Champagne +7 more
doaj +1 more source
From Clusters to Proto-Clusters: The Infrared Perspective on Environmental Galaxy Evolution
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it can control the critical process of transforming galaxies from star forming to quiescent, commonly termed “quenching”. Despite its importance, however, we still do
Stacey Alberts, Allison Noble
doaj +1 more source
The gravitational collapse of triaxial protoclusters [PDF]
The collapse of ellipsoids to the formation of a caustic surface is followed. The subsequent collapse of pancakes in their planes is investigated.
More, James G. +2 more
openaire +1 more source
We present the spectroscopic confirmation of a protocluster at z = 7.88 behind the galaxy cluster Abell 2744 (hereafter A2744-z7p9OD). Using JWST NIRSpec, we find seven galaxies within a projected radius of 60 kpc.
Takahiro Morishita +41 more
doaj +1 more source
Protocluster discovery in tomographic Ly α forest flux maps [PDF]
18 pages, 12 ...
Stark, Casey W +3 more
openaire +4 more sources
Subclustering and Star Formation Efficiency in Three Protoclusters in the Central Molecular Zone
We present the highest-resolution (∼0 $\mathop{.}\limits^{^{\prime\prime} }$ 04) Atacama Large Millimeter/submillimeter Array 1.3 mm continuum observations so far of three massive star-forming clumps in the Central Molecular Zone (CMZ), namely 20 km s ...
Suinan Zhang +23 more
doaj +1 more source
MeerKAT observations of Herschel protocluster candidates
ABSTRACT High-redshift protoclusters consisting of dusty starbursts are thought to play an important role in galaxy evolution. Their dusty nature makes them bright in the far-infrared (FIR)/submm but difficult to find in optical/near-infrared (NIR) surveys.
Y Ding +11 more
openaire +2 more sources
MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters
We examine the quiescent fractions of massive galaxies in six z ≳ 3 spectroscopically confirmed protoclusters in the COSMOS field, one of which is newly confirmed and presented here. We report the spectroscopic confirmation of MAGAZ3NE J100143+023021 at $
Ian McConachie +18 more
doaj +1 more source
Dusty Galaxies In Protoclusters
Comparison of Herschel and Planck sources in large area surveys has revealed a pop- ulation of objects that appear to be galaxy clusters or protoclusters, many of whose members are undergoing massive starbursts. Followup studies confirm the likely clus- ter/protocluster nature of these sources.
Clements, David L, +2 more
openaire +1 more source

