Results 121 to 130 of about 159,574 (199)
The enhancement of rapidly quenched galaxies in distant clusters at
0.5
We investigate the relationship between environment and galaxy evolution in the redshift range $0.5 < z < 1.0$. Galaxy overdensities are selected using a Friends-of-Friends algorithm, applied to deep photometric data in the Ultra-Deep Survey (UDS) field. A study of the resulting stellar mass functions reveals clear differences between cluster and field
arxiv +1 more source
Rethinking the relation between human and nature: Insights from science fiction
Abstract Facing the accumulation of data that suggest near‐future dramatic changes in our way of life, current visions of transition are anchored in an incremental paradigm that excludes radical change. Using science fiction literature and cinema, this article aims to build such drastic change hypotheses and explore the political–ecological features of
Corinne Gendron, René Audet
wiley +1 more source
The role of DNA content in shaping chromatin architecture and gene expression
SUMMARY Whole‐genome duplication is an evolutionary force that drives speciation in all living kingdoms and is notably prevalent in plants. The evolutionary history of plants involved at least two genomic duplications that significantly expanded the plant morphology and physiology spectrum. Many important crops are polyploids, showing valuable features
Alfonso Carlos Barragán‐Rosillo+2 more
wiley +1 more source
Galaxy Quenching and Assembly: A Review
A review of observational and theoretical constraints on galaxy assembly and quenching.
openaire +3 more sources
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
The formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon , to investigate the issue. We select two massive star formation quenched S0s as our main
Seongbong Han+11 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
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
On the Origin of Quenched but Gas-rich Regions at Kiloparsec Scales in Nearby Galaxies
We use resolved spectroscopy from MaNGA to investigate the significance of both local and global properties of galaxies to the cessation of star formation at kpc scales.
Tao Jing, Cheng Li
doaj +1 more source
Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 Mpc
It is well known that almost all isolated dwarf galaxies are actively forming stars. We report the discovery of dw1322m2053 (nicknamed Hedgehog), an isolated quiescent dwarf galaxy at a distance of 2.40 ± 0.15 Mpc with a stellar mass of M _⋆ ≈ 10 ^5.8 M ...
Jiaxuan Li+3 more
doaj +1 more source