Results 171 to 180 of about 495,355 (288)
A massive quiescent galaxy at redshift 4.658. [PDF]
Nature, 2023 Carnall AC +12 more
europepmc +1 more source
The Astrophysical JournalThe tight relationship between the stellar mass and halo mass of galaxies is one of the most fundamental scaling relations in galaxy formation and evolution. It has become a critical constraint for galaxy formation models.
Kai Wang, Yingjie Peng
doaj +1 more source
Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2 [PDF]
, 2017 Moein Mosleh +7 more
openalex +1 more source
A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters [PDF]
, 2020 Kyle A. Oman +5 more
openalex +1 more source
Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle [PDF]
, 2022 J. Davies +2 more
openalex +1 more source
, 2017 Peng et al. (2015, Nature, 521, 192) analysed stellar metallicities of 26,000 SDSS galaxies and found that galaxies with stellar masses below 1011 solar masses are primarily quenched due to the halting of the supply of cold gas (strangulation). We take this analysis further by making use of the much larger spectroscopic sample of galaxies in SDSS DR7 ...
Daniel Thomas +5 more
openaire +2 more sources
What is the right way to quench star formation in semi-analytic models of galaxy formation? [PDF]
, 2017 Yu Luo, Xi Kang
openalex +1 more source
The age gradients of galaxies in EAGLE: outside-in quenching as the origin of young bulges in cluster galaxies [PDF]
, 2022 Joel Pfeffer +4 more
openalex +1 more source
Active Galactic Nuclei in the Green Valley at z ∼ 0.7
The Astrophysical JournalWe present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( $\mathrm{log}\ {M}_{* }/{M}_{\odot }\gtrsim 10$ ) at z ∼ 0.7 with optical spectroscopy from the Large Early Galaxy ...
Charity Woodrum +7 more
doaj +1 more source