Results 11 to 20 of about 495,355 (288)

What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
We develop a 2D inclined rotating disc model, which we apply to the stellar velocity maps of 1862 galaxies taken from the MaNGA survey (SDSS public Data Release 15).
Simcha Brownson   +3 more
semanticscholar   +5 more sources

Rapid Quenching of Galaxies at Cosmic Noon

open access: yesThe Astrophysical Journal, 2023
The existence of massive quiescent galaxies at high redshift seems to require rapid quenching, but it is unclear whether all quiescent galaxies have gone through this phase and what physical mechanisms are involved.
Minjung Park   +8 more
doaj   +6 more sources

Both starvation and outflows drive galaxy quenching [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
Star-forming galaxies can in principle be transformed into passive systems by a multitude of processes that quench star formation, such as the halting of gas accretion (starvation) or the rapid removal of gas in AGN-driven outflows. However, it remains
J. Trussler   +6 more
semanticscholar   +7 more sources

Probing Satellite Quenching With Galaxy Clustering [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
Satellites within simulated massive clusters are significantly spatially correlated with each other, even when those satellites are not gravitationally bound to each other.
Chamberlain, Robert T.   +3 more
core   +4 more sources

The First Quenched Galaxies: When and How?

open access: yesThe Astrophysical Journal Letters
Many quiescent galaxies discovered in the early Universe by JWST raise fundamental questions on when and how these galaxies became and stayed quenched. Making use of the latest version of the semianalytic model GAEA that provides good agreement with the ...
Lizhi Xie   +13 more
doaj   +3 more sources

THE MASS DEPENDENCE OF DWARF SATELLITE GALAXY QUENCHING [PDF]

open access: yesThe Astrophysical Journal, 2014
We combine observations of the Local Group with data from the NASA-Sloan Atlas to show the variation in the quenched fraction of satellite galaxies from low-mass dwarf spheroidals and dwarf irregulars to more massive dwarfs similar to the Magellanic ...
C. Slater, E. Bell
semanticscholar   +5 more sources

The impact of quenching on galaxy profiles in the simba simulation [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
We study specific star formation rate (sSFR) and gas profiles of star forming and green valley galaxies in the Simba cosmological hydrodynamic simulation. Star-forming galaxy half-light radii ($R_{\rm half}$) at $z=0$ and their evolution ($\propto(1+z)^{-
S. Appleby   +4 more
semanticscholar   +7 more sources

Star formation quenching in massive galaxies [PDF]

open access: greenNature 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.
Allison W. S. Man, Sirio Belli
openalex   +5 more sources

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

open access: bronzeThe 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.
Anna K. Weigel   +11 more
openalex   +9 more sources

A dichotomy in satellite quenching around L* galaxies [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2013
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   +7 more sources

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