Results 1 to 10 of about 159,862 (240)
A STELLAR MASS THRESHOLD FOR QUENCHING OF FIELD GALAXIES [PDF]
We demonstrate that dwarf galaxies (10^7 < M_stellar < 10^9 Msun) with no active star formation are extremely rare (<0.06%) in the field. Our sample is based on the NASA-Sloan Atlas which is a re-analysis of the Sloan Digital Sky Survey Data Release 8.
Marla Geha+3 more
arxiv +6 more sources
A dichotomy in satellite quenching around L* galaxies [PDF]
We examine the star formation properties of bright (~0.1 L*) satellites around isolated ~L* hosts in the local Universe using spectroscopically confirmed systems in the Sloan Digital Sky Survey DR7. Our selection method is carefully designed with the aid of N-body simulations to avoid groups and clusters.
John I. Phillips+5 more
openalex +6 more sources
The formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon , to investigate the issue. We select two massive star formation quenched S0s as our main
Seongbong Han+11 more
doaj +1 more source
Environment plays a critical role in shaping the assembly of low-mass galaxies. Here, we use the U niverse M achine (UM) galaxy–halo connection framework and Data Release 3 of the Satellites Around Galactic Analogs (SAGA) Survey to place dwarf galaxy ...
Yunchong Wang+13 more
doaj +1 more source
Galaxy Bulges and their Black Holes: a Requirement for the Quenching of Star Formation [PDF]
Eric F. Bell
openalex +1 more source
On the Origin of Quenched but Gas-rich Regions at Kiloparsec Scales in Nearby Galaxies
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
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 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
CONFRONTING MODELS OF DWARF GALAXY QUENCHING WITH OBSERVATIONS OF THE LOCAL GROUP [PDF]
Colin T. Slater, Eric F. Bell
openalex +1 more source
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