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Gaseous galaxy halos
Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy's disk and
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …
Cold gas accretion in galaxies
Evidence for the accretion of cold gas in galaxies has been rapidly accumulating in the past
years. HI observations of galaxies and their environment have brought to light new facts and …
years. HI observations of galaxies and their environment have brought to light new facts and …
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 massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang
Cosmological models predict that galaxies forming in the early Universe experience a
chaotic phase of gas accretion and star formation, followed by gas ejection due to feedback …
chaotic phase of gas accretion and star formation, followed by gas ejection due to feedback …
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 …
MHONGOOSE: A MeerKAT nearby galaxy H i survey
WJG de Blok, J Healy, FM Maccagni, DJ Pisano… - Astronomy & …, 2024 - aanda.org
The MHONGOOSE (MeerKAT HI Observations of Nearby Galactic Objects: Observing
Southern Emitters) survey maps the distribution and kinematics of the neutral atomic …
Southern Emitters) survey maps the distribution and kinematics of the neutral atomic …
Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
We study the dynamics of cold molecular gas in two main-sequence galaxies at cosmic
noon (zC-488879 at z≃ 1.47 and zC-400569 at z≃ 2.24) using new high-resolution ALMA …
noon (zC-488879 at z≃ 1.47 and zC-400569 at z≃ 2.24) using new high-resolution ALMA …
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 …
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 () …
MIGHTEE-HI: The H i emission project of the MeerKAT MIGHTEE survey
We present the HI emission project within the MIGHTEE survey, currently being carried out
with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind …
with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind …