Results 41 to 50 of about 624,561 (255)
Accelerated Galaxy Growth and Environmental Quenching in a Protocluster at z = 3.24 [PDF]
Astrophysical Journal, 2021 We present a multiwavelength study of galaxies around D4UD01, a spectroscopically confirmed protocluster at z = 3.24, to investigate environmental trends. 450 galaxies are selected based on K S band detection with photometric redshifts (photo-z) at 3.0 <
Ke Shi +5 more
semanticscholar +1 more source
Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
The Astrophysical Journal, 2023 We explore how the fraction of quenched galaxies changes in groups of galaxies with respect to the distance to the center of the group, redshift, and stellar mass to determine the dominant process of environmental quenching in 0.2 < z < 0.8 groups.
Bonnabelle Zabelle +38 more
doaj +1 more source
MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching [PDF]
Astrophysical Journal, 2018 We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5 < z < 2.5 using deep rest-frame optical spectra obtained with Keck MOSFIRE.
S. Belli, A. Newman, R. Ellis
semanticscholar +1 more source
CLEAR: The Morphological Evolution of Galaxies in the Green Valley
The Astrophysical Journal, 2023 Quiescent galaxies having more compact morphologies than star-forming galaxies has been a consistent result in the field of galaxy evolution. What is not clear is at what point this divergence happens, i.e., when do quiescent galaxies become compact, and
Vicente Estrada-Carpenter +10 more
doaj +1 more source
Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in the Local Universe [PDF]
Astrophysical Journal, 2021 The phenomenological study of evolving galaxy populations in Peng et al. has shown that star forming galaxies can be quenched by two distinct processes: mass quenching and environment quenching. To explore the mass quenching process in local galaxies, we
Chengpeng Zhang +15 more
semanticscholar +1 more source
Quenching and Galaxy Demographics
, 2021 6 pages, 3 ...
de la Bella, Lucia F. +4 more
openaire +2 more sources
AGN-driven quenching of satellite galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 ABSTRACT We explore the effect of active galactic nucleus (AGN) feedback from central galaxies on their satellites by comparing two sets of cosmological zoom-in runs of 27 haloes with masses ranging from 1012 to 1013.4$\rm {M}_{\odot}$ at z = 0, with (wAGN) and without (noAGN) AGN feedback.
Jeremiah P. Ostriker +9 more
openaire +3 more sources
Bar quenching in gas-rich galaxies [PDF]
Astronomy & Astrophysics, 2018 Galaxy surveys have suggested that rapid and sustained decrease in the star-formation rate (SFR), “quenching”, in massive disk galaxies is frequently related to the presence of a bar. Optical and near-IR observations reveal that nearly 60% of disk galaxies in the local universe are barred, thus it is important to understand the relationship between ...
Khoperskov, S. +4 more
openaire +6 more sources
The Roles of Mass and Environment in the Quenching of Galaxies [PDF]
The Astrophysical Journal, 2019 Abstract We study the roles of stellar mass and environment in quenching the star formation activity of a large set of simulated galaxies by taking advantage of an analytic model coupled to the merger tree extracted from an N-body simulation. The analytic model has been set to match the evolution of the global stellar mass function since
E. Contini +5 more
openaire +6 more sources
Quenching star formation in cluster galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 In order to understand the processes that quench star formation within rich clusters, we construct a library of subhalo orbits drawn from $ $CDM cosmological N-body simulations of four rich clusters. The orbits are combined with models of star formation followed by quenching in the cluster environment.
Michael L. Balogh +10 more
openaire +4 more sources