Results 11 to 20 of about 350 (188)

Environmental quenching of low-mass field galaxies. [PDF]

open access: yesMon Not R Astron Soc, 2018
In the local Universe, there is a strong division in the star-forming properties of low-mass galaxies, with star formation largely ubiquitous amongst the field population while satellite systems are predominantly quenched. This dichotomy implies that environmental processes play the dominant role in suppressing star formation within this low-mass ...
Fillingham SP   +5 more
europepmc   +7 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

Galaxy Zoo: Major Galaxy Mergers Are Not a Significant Quenching Pathway* [PDF]

open access: yesThe Astrophysical Journal, 2017
Abstract We use stellar mass functions to study the properties and the significance of quenching through major galaxy mergers. In addition to SDSS DR7 and Galaxy Zoo 1 data, we use samples of visually selected major galaxy mergers and post-merger galaxies.
Weigel, A   +11 more
openaire   +5 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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