Results 131 to 140 of about 9,154 (212)
Restricted by event horizon suppression, tidal disruption events (TDEs) provide a unique window into otherwise hidden supermassive black holes (SMBHs) at the lower end of the mass spectrum, allowing the connection between star formation and SMBH mass to ...
Paige Ramsden +2 more
doaj +1 more source
The mystery of unidentified infrared emission bands. [PDF]
Kwok S.
europepmc +1 more source
Galaxy Quenching and Assembly: A Review
A review of observational and theoretical constraints on galaxy assembly and quenching.
openaire +1 more source
Environment plays a critical role in shaping the assembly of low-mass galaxies. Here, we use the U niverse M achine (UM) galaxy–halo connection framework and Data Release 3 of the Satellites Around Galactic Analogs (SAGA) Survey to place dwarf galaxy ...
Yunchong Wang +13 more
doaj +1 more source
Mechanisms for quenching star formation in galaxies remain hotly debated, with galaxy mergers an oft-proposed pathway. In Ellison et al. (2022) we tested this scenario by quantifying the fraction of recently and rapidly quenched post-starbursts (PSBs) in
Sara Ellison +5 more
doaj +1 more source
PAC. V. The Roles of Mass and Environment in the Quenching of Galaxies
The roles that mass and environment play in galaxy quenching are still under debate. Leveraging the Photometric objects Around Cosmic webs method, we analyze the excess surface distribution ${\bar{n}}_{2}{w}_{{\rm{p}}}({r}_{{\rm{p}}})$ of photometric ...
Yun Zheng +8 more
doaj +1 more source
The connection between dusty star-forming galaxies and the first massive quenched galaxies
High-redshift (z ≳ 2) massive quiescent galaxies (MQs) provide an opportunity to probe the key physical processes driving the fuelling and quenching of star formation in the early Universe.
Araya-Araya Pablo +8 more
doaj +1 more source
The Role of Gas Stripping in the Quenching of Satellite Galaxies Using SHARK v2.0
Observational studies have made substantial progress in characterizing quenching as a function of galaxy stellar mass and environment, but they are often limited in their ability to constrain quenching timescales and to determine the dominant ...
Megan K. Oxland +3 more
doaj +1 more source
Quenching of galaxies at cosmic noon
Context. We identified and analysed massive quiescent galaxies (MQGs) at z ≈ 3.1 within the 2 deg2 COSMOS field and explored the effect of the galaxy environment on quenching processes. By examining the variation in the quenched fraction and physical properties of these galaxies in different environmental contexts, including local densities ...
Akriti Singh +18 more
openaire +2 more sources
Merger Shocks Enhance Quenching in Local Galaxy Clusters
Abstract We report evidence for enhanced quenching in low-redshift galaxy clusters hosting radio relics. This effect is strongest for low-mass galaxies and is consistent with a rapid quenching of star formation. These results imply that merger shocks in the intracluster medium play a role in driving environmental quenching, which we ...
openaire +4 more sources

