Photodissociation and X-Ray-Dominated Regions
MG Wolfire, L Vallini, M Chevance - Annual Review of …, 2022 - annualreviews.org
The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
Cool outflows in galaxies and their implications
Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
A survey of high-z galaxies: serra simulations
We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7
L Sommovigo, A Ferrara, A Pallottini… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …
of galaxies in the Universe. However, the dust temperature T d remains mostly …
Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies' interstellar medium
We combine results from deep ALMA observations of massive (M*> 10 10 M⊙) galaxies at
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …
The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7
We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
High-redshift star formation in the Atacama large millimetre/submillimetre array era
JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
The ALPINE-ALMA [CII] survey-Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4< z< 6
The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …
Dynamical properties of z ∼4.5 dusty star-forming galaxies and their connection with local early-type galaxies
F Rizzo, S Vegetti, F Fraternali… - Monthly Notices of the …, 2021 - academic.oup.com
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 …
The alpine–alma [c ii] survey: Multiwavelength ancillary data and basic physical measurements
AL Faisst, D Schaerer, BC Lemaux… - The Astrophysical …, 2020 - iopscience.iop.org
We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …