Results 41 to 50 of about 15,230 (253)
Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe [PDF]
, 2016 Central galaxies make up the majority of the galaxy population, including the majority of the quiescent population at $\mathcal{M}_* > 10^{10}\mathrm{M}_\odot$.
Hahn, ChangHoon +2 more
core +2 more sources
Bar quenching in gas-rich galaxies [PDF]
Astronomy & Astrophysics, 2018 Galaxy surveys have suggested that rapid and sustained decrease in the star-formation rate (SFR), “quenching”, in massive disk galaxies is frequently related to the presence of a bar. Optical and near-IR observations reveal that nearly 60% of disk galaxies in the local universe are barred, thus it is important to understand the relationship between ...
Khoperskov, S. +4 more
openaire +4 more sources
Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9 [PDF]
, 2017 Indexación: Web of Science; Scopus.We analyse the evolution of environmental quenching efficiency, the fraction of quenched cluster galaxies which would be star forming if they were in the field, as a function of redshift in 14 spectroscopically ...
Cooper, M.C. +9 more
core +1 more source
Bursting and quenching in satellite galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 ABSTRACT The difference in stellar metallicity between red and blue galaxies with the same mass constrains the time-scale over which red galaxies ceased to form stars. Here we investigate this constraint with the galics 2.0 semi-analytic model of galaxy formation.
Koutsouridou, I, Cattaneo, A
openaire +3 more sources
AGN quenching in simulated dwarf galaxies
, 2022 23 pages, 11 figures; submitted to ...
Sharma, Ray S. +4 more
openaire +2 more sources
, 2014 Recent observations suggested that star formation quenching in galaxies is related to galaxy structure. Here we propose a new mechanism to explain the physical origin of this correlation. We assume that while quiescent galaxies are maintained quenched by
Guo, Fulai
core +1 more source
Inside-out growth or inside-out quenching? clues from colour gradients of local galaxies [PDF]
, 2017 We constrain the spatial gradient of star formation history within galaxies using the colour gradients in NUV-u and u-i for a local spatially-resolved galaxy sample.
Blanton, Michael +3 more
core +3 more sources
The LEGA-C galaxy survey: Multiple quenching channels for quiescent galaxies at z ∼ 1
Astronomy & AstrophysicsAims. We analyzed the sizes and star formation histories (SFHs) of 2908 galaxies with M★ ≥ 109 M⊙ at 0.6
Nersesian Angelos +11 more
doaj +1 more source
, 2017 Recent studies suggest that the quenching properties of galaxies are correlated over several mega-parsecs. The large-scale "galactic conformity" phenomenon around central galaxies has been regarded as a potential signature of "galaxy assembly bias" or ...
Mandelbaum, Rachel, Zu, Ying
core +1 more source
Mapping stellar content to dark matter halos. II. Halo mass is the main driver of galaxy quenching
, 2015 We develop a simple yet comprehensive method to distinguish the underlying drivers of galaxy quenching, using the clustering and galaxy-galaxy lensing of red and blue galaxies in SDSS.
Mandelbaum, Rachel, Zu, Ying
core +2 more sources