Results 11 to 20 of about 14,680 (203)

The First Quenched Galaxies: When and How?

open access: yesThe Astrophysical Journal Letters
Many 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

Dissecting the Mass Quenching in TNG50: Galaxy Size Determines the Quenching Mode

open access: yesThe Astrophysical Journal
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
Haochen Jiang   +4 more
doaj   +3 more sources

Quenched Galaxies in Clusters of Galaxies and Their Outskirts [PDF]

open access: yesAstrophysical 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

Signatures of quenching in dwarf galaxies in local galaxy clusters [PDF]

open access: yesAstronomy & Astrophysics, 2021
17 pages, 16 figures, accepted for publication in A& ...
Janz, Joachim   +3 more
  +7 more sources

Quenching of satellite galaxies at the outskirts of galaxy clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
We find, using cosmological simulations of galaxy clusters, that the hot X-ray emitting intra-cluster medium (ICM) enclosed within the outer accretion shock extends out to $R_{\rm shock}\sim(2 - 3) R_{\rm vir}$, where $R_{\rm vir}$ is the standard virial radius of the halo.
Elad Zinger   +3 more
openaire   +2 more sources

The Morphological Transformation and the Quenching of Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract We study the morphological transformation from late types to early types and the quenching of galaxies with the seventh Data Release (DR7) of the Sloan Digital Sky Survey. Both early-type galaxies and late-type galaxies are found to have bimodal distributions on the star formation rate versus stellar mass diagram (lg SFR–lg M
Chenxu Liu   +3 more
openaire   +2 more sources

How to quench a galaxy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
Clarifications and added references; accepted for publication in ...
Pontzen, Andrew   +7 more
openaire   +4 more sources

Quenching and Galaxy Demographics

open access: yes, 2021
6 pages, 3 ...
de la Bella, Lucia F.   +4 more
openaire   +2 more sources

Quenching star formation in cluster galaxies [PDF]

open access: yesMonthly 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 $Λ$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

Overconsumption, outflows and the quenching of satellite galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2014
Abstract The baryon cycle of galaxies is a dynamic process involving the intake, consumption and ejection of vast quantities of gas. In contrast, the conventional picture of satellite galaxies has them methodically turning a large gas reservoir into stars until this reservoir is forcibly removed due to external ram pressure. This picture
McGee, S.L., Bower, R.G., Balogh, M.L.
openaire   +4 more sources

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