Dynamical properties of z ∼4.5 dusty star-forming galaxies and their connection with local early-type galaxies
There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …
combination of stellar feedback processes and gravitational instabilities driven by mergers …
A unified model for galactic discs: star formation, turbulence driving, and mass transport
We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
Turbulent Gas in Lensed Planck-selected Starbursts at z∼ 1–3.5
Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …
regions in the universe. Key aspects to these processes are the gas heating and cooling …
The Evolution and Origin of Ionized Gas Velocity Dispersion from z∼ 2.6 to z∼ 0.6 with KMOS3D∗
H Übler, R Genzel, E Wisnioski… - The Astrophysical …, 2019 - iopscience.iop.org
The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with
KMOS3D - IOPscience This site uses cookies. By continuing to use this site you agree to our …
KMOS3D - IOPscience This site uses cookies. By continuing to use this site you agree to our …
SDSS-IV MaNGA: Modeling the spectral line-spread function to subpercent accuracy
DR Law, KB Westfall, MA Bershady… - The Astronomical …, 2021 - iopscience.iop.org
Abstract The Sloan Digital Sky Survey IV Map** Nearby Galaxies at APO (MaNGA)
program has been operating from 2014 to 2020, and has now observed a sample of 9269 …
program has been operating from 2014 to 2020, and has now observed a sample of 9269 …
Dynamical characterization of galaxies up to z∼ 7
Context. The characterization of the dynamical state of galaxies up to z∼ 7 is crucial for
constraining the mechanisms that drive the mass assembly in the early Universe. However …
constraining the mechanisms that drive the mass assembly in the early Universe. However …
Disc settling and dynamical heating: histories of Milky Way-mass stellar discs across cosmic time in the FIRE simulations
F McCluskey, A Wetzel, SR Loebman… - Monthly Notices of …, 2024 - academic.oup.com
We study the kinematics of stars both at their formation and today within 14 Milky Way (MW)-
mass galaxies from the FIRE-2 cosmological zoom-in simulations. We quantify the relative …
mass galaxies from the FIRE-2 cosmological zoom-in simulations. We quantify the relative …
The ALMA-ALPAKA survey-II. Evolution of turbulence in galaxy disks across cosmic time: Difference between cold and warm gas
The gas in the interstellar medium (ISM) of galaxies is supersonically turbulent.
Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and …
Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and …
REBELS-25: Discovery of a dynamically cold disc galaxy at z= 7.31
LE Rowland, J Hodge, R Bouwens… - Monthly Notices of …, 2024 - academic.oup.com
We present high-resolution (arcsec= 710 pc) Atacama Large Millimetre/submillimetre Array
[C ii] 158 m and dust continuum follow-up observations of REBELS-25, a [C ii]-luminous () …
[C ii] 158 m and dust continuum follow-up observations of REBELS-25, a [C ii]-luminous () …
ALMA hints at the presence of turbulent disk galaxies at z> 5
Context. High-redshift galaxies are expected to be more turbulent than local galaxies
because of their smaller size and higher star formation and thus stronger feedback from star …
because of their smaller size and higher star formation and thus stronger feedback from star …