Results 121 to 130 of about 9,154 (212)
Dissecting the Mass Quenching in TNG50: Galaxy Size Determines the Quenching Mode
Abstract The diminishing of star formation is accompanied by size differentiating, as quiescent galaxies are more compact than star-forming galaxies (SFGs) at fixed stellar mass. In order to understand how galaxy quenching is related to galaxy sizes, we performed a demographic study of 46 massive quiescent central
Haochen Jiang +4 more
openaire +2 more sources
The JWST EXCELS Survey: Insights into the Nature of Quenching at Cosmic Noon
We study 24 massive quiescent galaxies with $\mathrm{log}{{M}}_{* }/{{M}}_{\odot }\gt 10$ at 1
Maya Skarbinski +21 more
doaj +1 more source
We report the discovery of three faint and ultrafaint dwarf galaxies—Sculptor A, Sculptor B, and Sculptor C—in the direction of NGC 300 ( D = 2.0 Mpc), a Large Magellanic Cloud–mass galaxy.
David J. Sand +20 more
doaj +1 more source
RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5
We present the number density of massive ( ${\mathrm{log}}({M}_{* }/{M}_{\odot })\gt 10.3$ ) quiescent galaxies at 2
Yunchong Zhang +23 more
doaj +1 more source
Isolated, low-mass galaxies provide the opportunity to assess the impact of reionization on their star formation histories (SFHs) without the ambiguity of environmental processes associated with massive host galaxies.
Kristen B. W. McQuinn +14 more
doaj +1 more source
The Environmental Quenching Mechanisms of Field Dwarf Galaxies
Field dwarf galaxies not actively forming stars are relatively rare in the local Universe, but are present in cosmological hydrodynamical simulations.
José A. Benavides +4 more
doaj +1 more source
A massive quiescent galaxy at redshift 4.658. [PDF]
Carnall AC +12 more
europepmc +1 more source
Excavating the Ruins: An Ancient z = 2.675 Galaxy Which Formed in the First 500 Myr
We present the analysis of an ancient galaxy at z = 2.675, which we dub “Eridu.” Simultaneously modeling the JWST/NIRSpec G140M and G235M spectra from the SMILES program and 0.4–25 μ m Hubble Space Telescope, JWST/NIRCam, and JWST/MIRI photometry from ...
Ian McConachie +16 more
doaj +1 more source
Environmental history of filament galaxies
Galaxy properties, such as stellar mass and star formation rate, correlate with their position within the cosmic web. Although galaxy properties can be correlated with a specific environment at a certain cosmic epoch, they may have experienced different ...
Zakharova D. +4 more
doaj +1 more source
The environments of the radio galaxy population in simba. [PDF]
Thomas N, Davé R.
europepmc +1 more source

