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Molecular Gas and the Star-Formation Process on Cloud Scales in Nearby Galaxies
E Schinnerer, AK Leroy - Annual Review of Astronomy and …, 2024 - annualreviews.org
Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …
The Physical Origin of the Stellar Initial Mass Function
Stars are among the most fundamental structures of our Universe. They comprise most of the
baryonic and luminous mass of galaxies; synthesize heavy elements; and inject mass …
baryonic and luminous mass of galaxies; synthesize heavy elements; and inject mass …
Introducing TIGRESS-NCR. I. Coregulation of the Multiphase Interstellar Medium and Star Formation Rates
Massive, young stars are the main source of energy that maintains multiphase structure and
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …
Cosmic-ray acceleration of galactic outflows in multiphase gas
We investigate the dynamical interaction between cosmic rays (CRs) and the multiphase
interstellar medium (ISM) using numerical magnetohydrodynamic (MHD) simulations with a …
interstellar medium (ISM) using numerical magnetohydrodynamic (MHD) simulations with a …
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 …
Formation of a low-mass galaxy from star clusters in a 600-million-year-old Universe
The most distant galaxies detected were seen when the Universe was a scant 5% of its
current age. At these times, progenitors of galaxies such as the Milky Way were about …
current age. At these times, progenitors of galaxies such as the Milky Way were about …
The ALMaQUEST Survey XI: a strong but non-linear relationship between star formation and dynamical equilibrium pressure
We present the extended ALMA MaNGA QUEnching and STar formation survey
(ALMaQUEST), a combination of the original 46 ALMaQUEST galaxies plus new ALMA …
(ALMaQUEST), a combination of the original 46 ALMaQUEST galaxies plus new ALMA …
Metallicity dependence of pressure-regulated feedback-modulated star formation in the TIGRESS-NCR simulation suite
We present a new suite of numerical simulations of the star-forming interstellar medium
(ISM) in galactic disks using the TIGRESS-NCR framework. Distinctive aspects of our …
(ISM) in galactic disks using the TIGRESS-NCR framework. Distinctive aspects of our …
FEASTS Combined with Interferometry. I. Overall Properties of Diffuse H i and Implications for Gas Accretion in Nearby Galaxies
We present a statistical study of the properties of diffuse H i in 10 nearby galaxies,
comparing the H i detected by the single-dish telescope FAST (FEASTS program) and the …
comparing the H i detected by the single-dish telescope FAST (FEASTS program) and the …
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 …