Results 131 to 140 of about 15,230 (253)

The Structure and Formation Histories of Low-mass Quiescent Galaxies in the A2744 Cluster Environment

open access: yesThe Astrophysical Journal
Low-mass quiescent galaxies are thought to predominantly reside in overdense regions, as environmental effects are often invoked to explain their shutdown of star formation. These longer-timescale quenching mechanisms—such as interactions with hot gas in
Sam E. Cutler   +23 more
doaj   +1 more source

On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0–2.5 [PDF]

open access: bronze, 2019
Jorge A. Zavala   +12 more
openalex   +1 more source

Galaxy Quenching and Assembly: A Review

open access: yes, 2019
A review of observational and theoretical constraints on galaxy assembly and quenching.
openaire   +1 more source

DISCOVERY OF MASSIVE, MOSTLY STAR FORMATION QUENCHED GALAXIES WITH EXTREMELY LARGE Ly α EQUIVALENT WIDTHS AT z ∼ 3 [PDF]

open access: bronze, 2015
Yoshiaki Taniguchi   +23 more
openalex   +1 more source

On the Origin of Quenched but Gas-rich Regions at Kiloparsec Scales in Nearby Galaxies

open access: yesThe Astrophysical Journal
We use resolved spectroscopy from MaNGA to investigate the significance of both local and global properties of galaxies to the cessation of star formation at kpc scales.
Tao Jing, Cheng Li
doaj   +1 more source

Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 Mpc

open access: yesThe Astrophysical Journal Letters
It is well known that almost all isolated dwarf galaxies are actively forming stars. We report the discovery of dw1322m2053 (nicknamed Hedgehog), an isolated quiescent dwarf galaxy at a distance of 2.40 ± 0.15 Mpc with a stellar mass of M _⋆ ≈ 10 ^5.8 M ...
Jiaxuan Li   +3 more
doaj   +1 more source

The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing

open access: yesThe Astrophysical Journal
Xu & Jing reported a monotonic relationship between the host halo mass M _h and the morphology of massive central galaxies, characterized by the Sérsic index n , at fixed stellar mass, suggesting that morphology could serve as a good secondary proxy for ...
Zhenjie Liu   +4 more
doaj   +1 more source

A massive quiescent galaxy at redshift 4.658. [PDF]

open access: yesNature, 2023
Carnall AC   +12 more
europepmc   +1 more source

Near-ultraviolet signatures of environment-driven galaxy quenching in Sloan Digital Sky Survey groups [PDF]

open access: green, 2016
Jacob P. Crossett   +4 more
openalex   +1 more source

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