[C ii] Emission in a Self-regulated Interstellar Medium
A Gurman, CY Hu, A Sternberg… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The [C ii] 157.74 μm fine-structure transition is one of the brightest and most well-
studied emission lines in the far-infrared, produced in the interstellar medium (ISM) of …
studied emission lines in the far-infrared, produced in the interstellar medium (ISM) of …
GMF G214. 5-1.8 as traced by CO: I–cloud-scale CO freeze-out as a result of a low cosmic-ray ionization rate
SD Clarke, VA Makeev… - Monthly Notices of …, 2024 - academic.oup.com
We present an analysis of the outer Galaxy giant molecular filament (GMF) G214. 5-1.8
(G214. 5) using IRAM 30m data of 12CO, 13CO, and C18O. We find that the 12CO (1-0) and …
(G214. 5) using IRAM 30m data of 12CO, 13CO, and C18O. We find that the 12CO (1-0) and …
The origin and evolution of the [CII] deficit in HII regions and star-forming molecular clouds
Aims. We analyse synthetic emission maps of the [CII] 158 µm line and far-infrared (FIR)
continuum of simulated molecular clouds (MCs) within the SILCC-Zoom project to study the …
continuum of simulated molecular clouds (MCs) within the SILCC-Zoom project to study the …
Cloud properties across spatial scales in simulations of the interstellar medium
T Colman, N Brucy, P Girichidis, SCO Glover… - Astronomy & …, 2024 - aanda.org
Context. Molecular clouds (MCs) are structures of dense gas in the interstellar medium (ISM)
that extend from ten to a few hundred parsecs and form the main gas reservoir available for …
that extend from ten to a few hundred parsecs and form the main gas reservoir available for …
Observing the LMC with APEX: Signatures of large-scale feedback in the molecular clouds of 30 Doradus
K Grishunin, A Weiss, D Colombo, M Chevance… - Astronomy & …, 2024 - aanda.org
Context. Stellar feedback plays a crucial role in star formation and the life cycle of molecular
clouds. The intense star formation region 30 Doradus, which is located in the Large …
clouds. The intense star formation region 30 Doradus, which is located in the Large …
Atomic and molecular gas as traced by [C II] emission
B Casavecchia, U Maio, C Péroux, B Ciardi - Astronomy & Astrophysics, 2025 - aanda.org
The latest ALMA and JWST observations provide new information on the birth and evolution
of galaxies in the early Universe at the epoch of reionization. Measurements at redshift z> 5 …
of galaxies in the early Universe at the epoch of reionization. Measurements at redshift z> 5 …
How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
E Batziou, UP Steinwandel, K Dolag… - arXiv preprint arXiv …, 2024 - arxiv.org
In cosmological simulations of large-scale structure star formation and feedback in galaxies
are modelled by so-called sub-grid models, that represent a physically motivated …
are modelled by so-called sub-grid models, that represent a physically motivated …