Results 1 to 10 of about 14,200 (174)
Galaxy Quenching from Cosmic Web Detachment [PDF]
We propose the Cosmic Web Detachment (CWD) model, a framework to interpret the star-formation history of galaxies in a cosmological context. The CWD model unifies several starvation mechanisms known to disrupt or stop star formation into one single ...
Miguel A. Aragon Calvo+2 more
doaj +6 more sources
Mapping stellar content to dark matter halos. II. Halo mass is the main driver of galaxy quenching [PDF]
We develop a simple yet comprehensive method to distinguish the underlying drivers of galaxy quenching, using the clustering and galaxy-galaxy lensing of red and blue galaxies in SDSS.
Mandelbaum, Rachel, Zu, Ying
core +3 more sources
A Dichotomy in Satellite Quenching Around L* Galaxies [PDF]
We examine the star formation properties of bright (~0.1 L*) satellites around isolated ~L* hosts in the local Universe using spectroscopically confirmed systems in the Sloan Digital Sky Survey DR7. Our selection method is carefully designed with the aid
Boylan-Kolchin, Michael+5 more
core +3 more sources
We extend the phenomenological study of the evolving galaxy population of Peng et al (2010) to the central/satellite dichotomy in Yang et al. SDSS groups.
Carollo, Marcella+3 more
core +2 more sources
Star formation quenching in massive galaxies [PDF]
Understanding how and why star formation turns off in massive galaxies is a major challenge for studies of galaxy evolution. Many theoretical explanations have been proposed, but a definitive consensus is yet to be reached.Comment: Comment published in ...
Belli, Sirio, Man, Allison
core +2 more sources
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
We identify the intrinsic dependence of star formation quenching on a variety of galactic and environmental parameters, utilizing a machine-learning approach with Random Forest classification.
Asa F. L. Bluck+2 more
doaj +1 more source
We investigate the fraction of quenched satellite galaxies in host galaxy groups and clusters using TNG300 in the IllustrisTNG cosmological magnetohydrodynamical simulations.
So-Myoung Park+7 more
doaj +1 more source
Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
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
CLEAR: The Morphological Evolution of Galaxies in the Green Valley
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