THE MASS DEPENDENCE OF DWARF SATELLITE GALAXY QUENCHING [PDF]
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 +6 more sources
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
Galaxy Zoo: Major Galaxy Mergers Are Not a Significant Quenching Pathway* [PDF]
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. We determine the stellar mass functions of the stages that we would expect major merger quenched galaxies ...
Anna K. Weigel+11 more
arxiv +10 more sources
The quenching time scale and quenching rate of galaxies [PDF]
The average star formation rate (SFR) in galaxies has been declining since redshift of 2. A fraction of galaxies quench and become quiescent. We constrain two key properties of the quenching process: the quenching time scale and the quenching rate among galaxies.
Jianhui Lian+3 more
arxiv +6 more sources
Estimation of the Galaxy Quenching Rate in the Illustris Simulation [PDF]
Quenching is a key topic in exploring the formation and evolution of galaxies. In this work, we study the quenching rate, i.e., the variation in the fraction of quenched galaxies per unit time, of the Illustris-1 simulation.
Yang Wang+4 more
semanticscholar +2 more sources
Rapid Quenching of Galaxies at Cosmic Noon
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
What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe [PDF]
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
Galaxy Quenching with Mass Growth History of Galaxy Groups and Clusters: The Importance of Post-processing [PDF]
We investigate the fraction of quenched satellite galaxies in host galaxy groups and clusters using TNG300 in the IllustrisTNG cosmological magnetohydrodynamical simulations.
So-Myoung Park+7 more
doaj +2 more sources
Filaments in VIPERS: galaxy quenching in the infalling regions of groups [PDF]
We study the quenching of galaxies in different environments and its evolution in the redshift range $0.43 \leq z \leq 0.89$. For this purpose, we identify galaxies inhabiting filaments, the isotropic infall region of groups, the field, and groups in the
J. M. Salerno, H. Mart'inez, H. Muriel
semanticscholar +2 more sources
Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation [PDF]
A rare population of massive disk galaxies have been found to invade the red sequence dominated by early-type galaxies. These red/quenched massive disk galaxies have recently gained great interest into their formation and origins. The usually proposed quenching mechanisms, such as bar quenching and environment quenching, seem not suitable for those ...
Yingzhong 迎中 Xu 徐+6 more
arxiv +5 more sources