Results 41 to 50 of about 188 (137)
Formation of Protoclusters in the Tank Industry of the Urals in 1941–1945 [PDF]
The article considers the process of the formation of the tank industry in the Urals during the Great Patriotic War in connection with the aspects of regional development within the large territorial and industrial entities. In modern economic science,
Vladimir Vasilyevich Zapariy +2 more
doaj +1 more source
Probing the effect of the protocluster environment on galaxy morphology at z = 2.23
Context. As galaxies evolve in dense cluster and protocluster environments, they interact and quench their star formation. This gradually transforms the dominant galaxy population from star-forming galaxies to quiescent red galaxies.
Golden-Marx E. +9 more
doaj +1 more source
Enhancement of AGN in a protocluster at z = 1.6 [PDF]
9 pages, 8 figures, Accepted to MNRAS (24th May 2017)
Charutha Krishnan +9 more
openaire +5 more sources
ODIN: High Clustering Strength of Protoclusters at Cosmic Noon
The One-hundred-deg ^2 DECam Imaging in Narrowbands (ODIN) survey is carrying out a systematic search for protoclusters during Cosmic Noon, using Ly α -emitting galaxies (LAEs) as tracers.
Vandana Ramakrishnan +19 more
doaj +1 more source
We present a high-angular resolution (∼1″) and wide-field ( $2\buildrel{\,\prime}\over{.} 9\times 1\buildrel{\,\prime}\over{.} 9$ ) image of the 1.3 mm continuum, CO( J = 2–1) and SiO( J = 5–4) line emissions toward an embedded protocluster, FIR 3, FIR 4,
Asako Sato +8 more
doaj +1 more source
ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Lyα-emitting Galaxies
To understand the formation and evolution of massive cosmic structures, studying them at high redshift, in the epoch when they formed the majority of their mass, is essential.
Vandana Ramakrishnan +26 more
doaj +1 more source
The realm of the galaxy protoclusters [PDF]
Reference corrected and text updated to match published ...
openaire +3 more sources
We investigate the consistency of intergalactic medium (IGM) tomography and galaxy surveys as tracers of the cosmic web and protoclusters at z ∼ 2.5. We use maps from the Ly α Tomography IMACS Survey (LATIS), which trace the distributions of Lyman-break
Andrew B. Newman +13 more
doaj +1 more source
Protocluster survey/characterization with NGRST
Protoclusters are interesting laboratories of galaxy evolution. To study their typical properties, first of all, deep and wide surveys are required since their surface density is quite small (a few in deg^2). Based on the deep and wide survey in optical by Hyper Suprime-Cam Subaru Strategic Program, the largest (N=179 in 121 deg^2) and uniform catalog ...
openaire +1 more source
Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at z ≥ 10?
Recent photometric detections of extreme ( z > 10) redshift galaxies from the JWST have been shown to be in strong tension with existing simulation models for galaxy formation and in the most acute case, in tension with ΛCDM itself.
B. W. Keller +3 more
doaj +1 more source

