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
The cumulative star formation histories of dwarf galaxies with TNG50. I: environment-driven diversity and connection to quenching [PDF]
Gandhali D Joshi +7 more
openalex +1 more source
CAUGHT IN THE ACT: GAS AND STELLAR VELOCITY DISPERSIONS IN A FAST QUENCHING COMPACT STAR-FORMING GALAXY AT z ∼ 1.7 [PDF]
Guillermo Barro +22 more
openalex +1 more source
From large-scale environment to CGM angular momentum to star forming activities – II. Quenched galaxies [PDF]
Shengdong Lu +9 more
openalex +1 more source
The Importance of Gas Starvation in Driving Satellite Quenching in Galaxy Groups at z ~ 0.8
We present results from a Keck/DEIMOS survey to study satellite quenching in group environments at z ~ 0.8 within the Extended Groth Strip (EGS). We target 11 groups in the EGS with extended X-ray emission. We obtain high-quality spectroscopic redshifts
Devontae C. Baxter +3 more
doaj +1 more source
THE ISLANDS PROJECT. I. ANDROMEDA XVI, AN EXTREMELY LOW MASS GALAXY NOT QUENCHED BY REIONIZATION* [PDF]
M. Monelli +16 more
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DESI Massive Poststarburst Galaxies at z ∼ 1.2 Have Compact Structures and Dense Cores
Poststarburst galaxies (PSBs) are young quiescent galaxies that have recently experienced a rapid decrease in star formation, allowing us to probe the fast-quenching period of galaxy evolution.
Yunchong Zhang +36 more
doaj +1 more source
The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation [PDF]
Jamie R. Ownsworth +6 more
openalex +1 more source
The Environmental Quenching Mechanisms of Field Dwarf Galaxies
Abstract Field dwarf galaxies not actively forming stars are relatively rare in the local Universe, but are present in cosmological hydrodynamical simulations. We use the TNG50 simulation to investigate their origin and find that they all result from environmental effects that have removed or reduced their gas content.
José A. Benavides +4 more
openaire +4 more sources
Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVER
We present a measurement of the low-mass quiescent size–mass relation at cosmic noon (1 < z < 3) from the JWST PRIMER and UNCOVER treasury surveys, which highlights two distinct classes of quiescent galaxies.
Sam E. Cutler +33 more
doaj +1 more source

