Results 51 to 60 of about 497,560 (237)
The enhancement of rapidly quenched galaxies in distant clusters at 0.5 < z < 1.0 [PDF]
, 2018 Funding: MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild).
M. Socolovsky +9 more
semanticscholar +1 more source
Galaxy Quenching from Cosmic Web Detachment [PDF]
The Open Journal of Astrophysics, 2019 20 pages, accepted for publication in OJA.
Aragon-Calvo, Miguel A. +2 more
openaire +4 more sources
Signatures of quenching in dwarf galaxies in local galaxy clusters
Astronomy & Astrophysics, 2021 17 pages, 16 figures, accepted for publication in A& ...
Janz, Joachim +3 more
openaire +3 more sources
The Astrophysical Journal, 2023 The assembly of galaxies over cosmic time is tightly connected to the assembly of their host dark matter halos. We investigate the stellar mass growth history and the chemical enrichment history of central galaxies in the Sloan Digital Sky Survey Mapping
Cheqiu Lyu +14 more
doaj +1 more source
Morphology Dependence of Stellar Age in Quenched Galaxies at Redshift ∼1.2:Massive Compact Galaxies Are Older than More Extended Ones [PDF]
, 2016 We report the detection of morphology-dependent stellar age in massive quenched galaxies (QGs) at z ∼ 1.2. The sense of the dependence is that compact QGs are 0.5–2 Gyr older than normal-sized ones. The evidence comes from three different age indicators—
C. Williams +8 more
semanticscholar +1 more source
The Astrophysical Journal, 2023 Conformity denotes the correlation of properties between pairs of galaxies as a function of separation. Correlations between properties such as the star formation rate (SFR), stellar mass, and specific star formation rate (sSFR) have implications for the
Charlotte Olsen, Eric Gawiser
doaj +1 more source
Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 Mpc [PDF]
Astrophysical Journal Letters, 2022 We report the discovery of Tucana B, an isolated ultra-faint dwarf galaxy at a distance of D = 1.4 Mpc. Tucana B was found during a search for ultra-faint satellite companions to the known dwarfs in the outskirts of the Local Group, although its sky ...
D. Sand +9 more
semanticscholar +1 more source
Recently Quenched Galaxies at z = 0.2–4.8 in the COSMOS UltraVISTA Field [PDF]
, 2017 We present a new analysis of the stellar mass function and morphology of recently quenched galaxies (RQGs), whose star formation has been recently quenched for some reason.
Akie Ichikawa, Y. Matsuoka
semanticscholar +1 more source
The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics [PDF]
Monthly notices of the Royal Astronomical Society, 2018 We select galaxies from the IllustrisTNG hydrodynamical simulations ($M_{\rm stars}\gt 10^9 \, {\rm M}_\odot$ at 0 ≤ z ≤ 2) and characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass (SFR–Mstars) diagrams.
M. Donnari +8 more
semanticscholar +1 more source
Star formation quenching in massive galaxies [PDF]
Nature Astronomy, 2018 Understanding how and why star formation turns off in massive galaxies is a major challenge for studies of galaxy evolution. Many theoretical explanations have been proposed, but a definitive consensus is yet to be reached.
Man A., Belli S.
openaire +4 more sources