Results 21 to 30 of about 16,096,383 (218)

ODIN: Where Do Lyα Blobs Live? Contextualizing Blob Environments within Large-scale Structure

open access: yesThe Astrophysical Journal, 2023
While many Ly α blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Ly α emitters (LAEs) and 129 LABs at z =
Vandana Ramakrishnan   +18 more
doaj   +1 more source

The clustering and host haloes of galaxy mergers at high redshift [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
10 pages, 5 figures, accepted in MNRAS, version matches published ...
Wetzel, Andrew R.   +2 more
openaire   +2 more sources

Spatial clustering of high-redshift Lyman-break galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
Accepted for publication in ...
Jose, Charles   +3 more
openaire   +2 more sources

Clustering of galaxies at high redshifts [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1998
Recent observations show a large concentration of galaxies at high redshift. At first sight, strong clustering of galaxies at high redshifts seems to be in contradiction with the models of structure formation. In this paper we show that such structures are a manifestation of the strong clustering of rare peaks in the density field.
openaire   +1 more source

Methods for identifying high‐redshift galaxy cluster candidates [PDF]

open access: yesAstronomische Nachrichten, 2019
AbstractRecent theories linked long gamma ray bursts (GRBs) to galaxies with rapid star formation or starburst; thus, we expect that long GRBs (LGRBs) are more frequent in midcluster galaxies where mergers and tidal interactions between gas‐rich galaxies are more likely to occur. Yet there is no galaxy cluster known to be associated with LGRBs.
Pinter, Sandor   +5 more
openaire   +2 more sources

The Clustering of High‐Redshift Galaxies in the Cold Dark Matter Scenario [PDF]

open access: yesThe Astrophysical Journal, 1999
33 pages, 10 figures, AAS LaTeX (aaspp4.sty), submitted to ...
Katz, N, Hernquist, L, Weinberg, DH
openaire   +4 more sources

Accelerated Structural Evolution of Galaxies in a Starbursting Cluster at z = 2.51

open access: yesThe Astrophysical Journal Letters, 2023
Structural properties of cluster galaxies during their peak formation epoch, z ∼ 2–4 provide key information on whether and how the environment affects galaxy formation and evolution.
Can Xu   +13 more
doaj   +1 more source

The observed properties of high-redshift cluster galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1995
We use the semi-analytic models of galaxy formation developed by Kauffmann, White \& Guiderdoni to generate predictions for the observed properties of cluster and group galaxies at redshifts between 0 and 0.6. We examine four sets of cosmological initial conditions: low-density CDM models with and without cosmological constant, a flat CDM model and
openaire   +2 more sources

Implications of multiple high-redshift galaxy clusters [PDF]

open access: yesPhysical Review D, 2011
11 pages, 7 figures, modified to match published ...
Ben Hoyle, Raul Jimenez, Licia Verde
openaire   +3 more sources

A high redshift sample of x-ray selected galaxy clusters [PDF]

open access: yes, 1998
This thesis describes the creation of a X-ray selected galaxy cluster catalogue — the Southern Serendipitous High-redshift Archival ROSAT Cluster (SHARC) catalogue — and the use of the high-redshift subsample in constraining models of structure formation.
Burke, Douglas John
core   +4 more sources

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