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 …

Molecular clouds in the Milky Way

M Heyer, TM Dame - Annual Review of Astronomy and …, 2015 - annualreviews.org
In the past twenty years, the reconnaissance of 12CO and 13CO emission in the Milky Way
by single-dish millimeter-wave telescopes has expanded our view and understanding of …

ATLASGAL–properties of a complete sample of Galactic clumps

JS Urquhart, C König, A Giannetti… - Monthly Notices of …, 2018 - academic.oup.com
Abstract The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is an unbiased
870 μm submillimetre survey of the inner Galactic plane (| ℓ|< 60° with| b|< 1 5). It is the …

Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues-First data release for the inner Milky Way:+ 68°≥ l≥− 70°

S Molinari, E Schisano, D Elia, M Pestalozzi… - Astronomy & …, 2016 - aanda.org
Aims. We present the first public release of high-quality data products (DR1) from Hi-GAL,
the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum …

Dense molecular gas properties on 100 pc scales across the disc of NGC 3627

I Bešlić, AT Barnes, F Bigiel, J Puschnig… - Monthly Notices of …, 2021 - academic.oup.com
It is still poorly constrained how the densest phase of the interstellar medium varies across
galactic environment. A large observing time is required to recover significant emission from …

The Hi-GAL catalogue of dusty filamentary structures in the Galactic plane

E Schisano, S Molinari, D Elia… - Monthly Notices of …, 2020 - academic.oup.com
The recent data collected by Herschel have confirmed that interstellar structures with a
filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to be …

[HTML][HTML] SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

F Schuller, T Csengeri, JS Urquhart… - Astronomy & …, 2017 - aanda.org
Context. The origin and life-cycle of molecular clouds are still poorly constrained, despite
their importance for understanding the evolution of the interstellar medium. Many large-scale …

ATLASGAL: A Galaxy-wide sample of dense filamentary structures

GX Li, JS Urquhart, S Leurini, T Csengeri… - Astronomy & …, 2016 - aanda.org
Context. Filamentary structures are ubiquitous in the interstellar medium. Investigating their
connection to the large-scale structure of the Galaxy and their role in star formation is …

Gravitational collapse and accretion flows in the hub filament system G323. 46-0.08

Y Ma, J Zhou, J Esimbek, W Baan, D Li, X Tang… - Astronomy & …, 2023 - aanda.org
We studied the hub-filament system G323. 46-0.08 based on archival molecular line data
from the SEDIGISM 13 CO survey and infrared data from the GLIMPSE, MIPS, and Hi-GAL …

Supernova remnants interacting with molecular clouds: X-ray and gamma-ray signatures

P Slane, A Bykov, DC Ellison, G Dubner… - Space Science …, 2015 - Springer
The giant molecular clouds (MCs) found in the Milky Way and similar galaxies play a crucial
role in the evolution of these systems. The supernova explosions that mark the death of …