Dust, CO, and [C i]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
L Dunne, SJ Maddox, PP Papadopoulos… - Monthly Notices of …, 2022 - academic.oup.com
We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …
JWST reveals widespread AGN-driven neutral gas outflows in massive z ~ 2 galaxies
We use deep JWST/NIRSpec R∼ 1000 slit spectra of 113 galaxies at, selected from the
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …
xCOLD GASS: the complete IRAM 30 m legacy survey of molecular gas for galaxy evolution studies
A Saintonge, B Catinella, LJ Tacconi… - The Astrophysical …, 2017 - iopscience.iop.org
We introduce xCOLD GASS, a legacy survey providing a census of molecular gas in the
local universe. Building on the original COLD GASS survey, we present here the full sample …
local universe. Building on the original COLD GASS survey, we present here the full sample …
Cosmic ray processes in galactic ecosystems
Galaxy evolution is an important topic, and our physical understanding must be complete to
establish a correct picture. This includes a thorough treatment of feedback. The effects of …
establish a correct picture. This includes a thorough treatment of feedback. The effects of …
The merger fraction of post-starburst galaxies in UNIONS
Post-starburst galaxies (PSBs) are defined as having experienced a recent burst of star
formation, followed by a prompt truncation in further activity. Identifying the mechanism (s) …
formation, followed by a prompt truncation in further activity. Identifying the mechanism (s) …
ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z∼ 1.5
CC Williams, JS Spilker, KE Whitaker… - The Astrophysical …, 2021 - iopscience.iop.org
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies
at z ∼ 1.5 - IOPscience This site uses cookies. By continuing to use this site you agree to our …
at z ∼ 1.5 - IOPscience This site uses cookies. By continuing to use this site you agree to our …
Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs
E Sazonova, K Alatalo, K Rowlands… - The Astrophysical …, 2021 - iopscience.iop.org
How do galaxies transform from blue, star-forming spirals to red, quiescent early-type
galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst …
galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst …
Rapid quenching of galaxies at cosmic noon
M Park, S Belli, C Conroy, S Tacchella… - The Astrophysical …, 2023 - iopscience.iop.org
The existence of massive quiescent galaxies at high redshift seems to require rapid
quenching, but it is unclear whether all quiescent galaxies have gone through this phase …
quenching, but it is unclear whether all quiescent galaxies have gone through this phase …
Now You See It, Now You Don't: Star Formation Truncation Precedes the Loss of Molecular Gas by∼ 100 Myr in Massive Poststarburst Galaxies at z∼ 0.6
R Bezanson, JS Spilker, KA Suess… - The Astrophysical …, 2022 - iopscience.iop.org
We use ALMA observations of CO (2–1) in 13 massive (M*≳ 10 11 M⊙) poststarburst
galaxies at z∼ 0.6 to constrain the molecular gas content in galaxies shortly after they …
galaxies at z∼ 0.6 to constrain the molecular gas content in galaxies shortly after they …
The interstellar medium of quiescent galaxies and its evolution with time
We characterise the basic far-IR properties and the gas mass fraction of massive (⟨ log
(M*/M⊙)⟩≈ 11.0) quiescent galaxies (QGs) and explore how these evolve from z= 2.0 to …
(M*/M⊙)⟩≈ 11.0) quiescent galaxies (QGs) and explore how these evolve from z= 2.0 to …