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Galaxy Formation in ΛCDM Cosmology
JR Primack - Annual Review of Nuclear and Particle Science, 2024 - annualreviews.org
This is a golden age for galaxy formation: Existing and especially new telescopes are
providing observations that challenge and illuminate rapidly improving theory and …
providing observations that challenge and illuminate rapidly improving theory and …
EPOCHS VI: the size and shape evolution of galaxies since z ∼ 8 with JWST Observations
We present the results of a size and structural analysis of 1395 galaxies at 0.5≤ z≲ 8 with
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …
Evolution of the Size–Mass Relation of Star-forming Galaxies Since z= 5.5 Revealed by CEERS
E Ward, A de la Vega, B Mobasher… - The Astrophysical …, 2024 - iopscience.iop.org
We combine deep imaging data from the CEERS early release JWST survey and Hubble
Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming …
Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming …
The epoch of the Milky Way's bar formation: dynamical modelling of Mira variables in the nuclear stellar disc
JL Sanders, D Kawata, N Matsunaga… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT A key event in the history of the Milky Way is the formation of the bar. This event
affects the subsequent structural and dynamical evolution of the entire Galaxy. When the bar …
affects the subsequent structural and dynamical evolution of the entire Galaxy. When the bar …
Formation of Galactic Disks. I. Why Did the Milky Way's Disk Form Unusually Early?
Recent results from spectroscopic and astrometric surveys of nearby stars suggest that the
stellar disk of our Milky Way (MW) was formed quite early, within the first few billion years of …
stellar disk of our Milky Way (MW) was formed quite early, within the first few billion years of …
The ALMA-ALPAKA survey-I. High-resolution CO and [CI] kinematics of star-forming galaxies at z= 0.5–3.5
Context. Spatially resolved studies of the kinematics of galaxies provide crucial insights into
their assembly and evolution, enabling one to infer the properties of the dark matter halos …
their assembly and evolution, enabling one to infer the properties of the dark matter halos …
A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3
The presence of a stellar bar in a disc galaxy indicates that the galaxy hosts in its main part a
dynamically settled disc and that bar-driven processes are taking place in sha** its …
dynamically settled disc and that bar-driven processes are taking place in sha** its …
[HTML][HTML] Accelerated structure formation: The early emergence of massive galaxies and clusters of galaxies
Galaxies in the early Universe appear to have grown too big too fast, assembling into
massive, monolithic objects more rapidly than anticipated in the hierarchical Lambda cold …
massive, monolithic objects more rapidly than anticipated in the hierarchical Lambda cold …
Galaxy mergers in UNIONS–I. A simulation-driven hybrid deep learning ensemble for pure galaxy merger classification
Merging and interactions can radically transform galaxies. However, identifying these events
based solely on structure is challenging as the status of observed mergers is not easily …
based solely on structure is challenging as the status of observed mergers is not easily …
Galaxy quenching at the high redshift frontier: A fundamental test of cosmological models in the early universe with JWST-CEERS
We present an analysis of the quenching of star formation in massive galaxies (M*> 10 9.5
M⊙) within the first 0.5–3 Gyr of the Universe's history utilizing JWST-CEERS data. We …
M⊙) within the first 0.5–3 Gyr of the Universe's history utilizing JWST-CEERS data. We …