Results 81 to 90 of about 1,048 (176)
The Bryde's whale is one of the least understood baleen whale species globally, limiting accuracy of regional and global conservation assessment. This study shows the occurrence of unique genetic lineages and evolutionary histories among Bryde's whale populations.
Dominique Paynee +7 more
wiley +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
Comparing Inside-out and Outside-in Quenching Modes in MaNGA Observation and MaNGIA Simulation
This study probes the inside-out and outside-in quenching status of galaxies to understand the internal and external quenching sources responsible and their roles in galaxy evolution.
Hung-Yu Jian +7 more
doaj +1 more source
Galaxy Quenching and Assembly: A Review
A review of observational and theoretical constraints on galaxy assembly and quenching.
openaire +2 more sources
Spatially resolved stellar populations of massive quiescent galaxies at cosmic noon provide powerful insights into star-formation quenching and stellar mass assembly mechanisms.
Cheng Chloe M. +18 more
doaj +1 more source
We present the elemental abundances and ages of 19 massive quiescent galaxies at z ∼ 1.4 and z ∼ 2.1 from the Keck Heavy Metal Survey. The ultradeep LRIS and MOSFIRE spectra were modeled using a full-spectrum stellar population fitting code with variable
Aliza G. Beverage +13 more
doaj +1 more source
SDSS-C4 3028: the Nearest Blue Galaxy Cluster Devoid of an Intracluster Medium
SDSS-C4 3028 is a galaxy cluster at $z=0.061$, notable for its unusually high fraction of star-forming galaxies with 19 star-forming and 11 quiescent spectroscopically-confirmed member galaxies. From Subaru/HSC imaging, we derived a weak lensing mass of $
Shweta Jain +11 more
doaj +1 more source
Widespread Rapid Quenching at Cosmic Noon Revealed by JWST Deep Spectroscopy
Massive quiescent galaxies in the young Universe are expected to be quenched rapidly, but it is unclear whether they all experience starbursts before quenching and what physical mechanism drives rapid quenching. We study 14 massive quiescent galaxies ( $\
Minjung Park +18 more
doaj +1 more source
A Massive Quiescent Galaxy in a Group Environment at z = 4.53
We report on the spectroscopic confirmation of a massive quiescent galaxy at z _spec = 4.53 in the COSMOS field. The object was first identified as a galaxy with suppressed star formation at z _phot ∼ 4.65 from the COSMOS2020 catalog.
Takumi Kakimoto +12 more
doaj +1 more source
Star formation quenching precedes morphological transformation in COSMOS-Web’s richest galaxy groups
We analyzed the 25 richest galaxy groups in COSMOS-Web across the redshift range z = 0.18–3.65, identified using the Adaptive Matched Identifier of Clustered Objects (AMICO) algorithm.
Ghaffari Z. +28 more
doaj +1 more source

