Results 11 to 20 of about 14,525 (205)
Probing Satellite Quenching With Galaxy Clustering [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 Satellites within simulated massive clusters are significantly spatially correlated with each other, even when those satellites are not gravitationally bound to each other.
Chamberlain, Robert T. +3 more
core +3 more sources
Dissecting the Mass Quenching in TNG50: Galaxy Size Determines the Quenching Mode
The Astrophysical JournalThe 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
Haochen Jiang +4 more
doaj +3 more sources
The First Quenched Galaxies: When and How?
The Astrophysical Journal LettersMany quiescent galaxies discovered in the early Universe by JWST raise fundamental questions on when and how these galaxies became and stayed quenched. Making use of the latest version of the semianalytic model GAEA that provides good agreement with the ...
Lizhi Xie +13 more
doaj +3 more sources
Merger Shocks Enhance Quenching in Local Galaxy Clusters
The Astrophysical JournalWe report evidence for enhanced quenching in low-redshift galaxy clusters hosting radio relics. This effect is strongest for low-mass galaxies and is consistent with a rapid quenching of star formation.
Ian D. Roberts
doaj +4 more sources
Galaxy zoo: stronger bars facilitate quenching in star-forming galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACTWe have used Galaxy Zoo DECaLS (GZD) to study strong and weak bars in disc galaxies. Out of the 314 000 galaxies in GZD, we created a volume-limited sample (0.01 < z < 0.05, Mr < − 18.96) which contains 1867 galaxies with reliable volunteer bar classifications in the ALFALFA footprint.
Tobias Géron +6 more
openaire +2 more sources
Quenched Galaxies in Clusters of Galaxies and Their Outskirts [PDF]
Astrophysical Bulletin, 2020 Based on the SDSS data, the properties of galaxies with quenched star formation (QGs) within the "splashback"-radius of galaxy clusters $R_{\rm sp}$ and beyond it have been studied.
Kopylova, Flera G. +1 more
openaire +2 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.
Taranu, Dan S. +6 more
openaire +3 more sources
Multiple mechanisms quench passive spiral galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 15 pages, 7 figures, accepted for publication in ...
Fraser-McKelvie, Amelia +4 more
openaire +5 more sources
Quenching and Galaxy Demographics
, 2021 6 pages, 3 ...
de la Bella, Lucia F. +4 more
openaire +2 more sources
Environmental quenching of low-mass field galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 In the local Universe, there is a strong division in the star-forming properties of low-mass galaxies, with star formation largely ubiquitous amongst the field population while satellite systems are predominantly quenched. This dichotomy implies that environmental processes play the dominant role in suppressing star formation within this low-mass ...
Sean P Fillingham +5 more
openaire +5 more sources