The cold interstellar medium of galaxies in the local universe
A Saintonge, B Catinella - Annual Review of Astronomy and …, 2022 - annualreviews.org
The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …
Ram pressure strip** in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
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 …
PHIBSS: unified scaling relations of gas depletion time and molecular gas fractions
This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
Dusty star-forming galaxies at high redshift
Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
The lifecycle of molecular clouds in nearby star-forming disc galaxies
M Chevance, JMD Kruijssen… - Monthly Notices of …, 2020 - academic.oup.com
It remains a major challenge to derive a theory of cloud-scale (pc) star formation and
feedback, describing how galaxies convert gas into stars as a function of the galactic …
feedback, describing how galaxies convert gas into stars as a function of the galactic …
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 …
Tracing the total molecular gas in galaxies:[CII] and the CO-dark gas
Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …
often used to deduce the total molecular hydrogen but is challenging to detect in low …
Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range
A Rémy-Ruyer, SC Madden, F Galliano… - Astronomy & …, 2014 - aanda.org
Aims. The goal of this paper is to analyse the behaviour of the gas-to-dust mass ratio (G/D)
of local Universe galaxies over a wide metallicity range. We especially focus on the low …
of local Universe galaxies over a wide metallicity range. We especially focus on the low …
Molecular cloud populations in the context of their host galaxy environments: a multiwavelength perspective
We present a rich, multiwavelength, multiscale database built around the PHANGS–ALMA
CO (2− 1) survey and ancillary data. We use this database to present the distributions of …
CO (2− 1) survey and ancillary data. We use this database to present the distributions of …