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 …

The Hi-GAL compact source catalogue–II. The 360° catalogue of clump physical properties

D Elia, M Merello, S Molinari, E Schisano… - Monthly Notices of …, 2021 - academic.oup.com
We present the 360° catalogue of physical properties of Hi-GAL compact sources, detected
between 70 and 500 m. This release not only completes the analogous catalogue previously …

ATLASGAL–evolutionary trends in high-mass star formation

JS Urquhart, MRA Wells, T Pillai… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT ATLASGAL is an 870-µm dust survey of 420 deg2 the inner Galactic plane and
has been used to identify∼ 10 000 dense molecular clumps. Dedicated follow-up …

[HTML][HTML] CoCCoA: Complex Chemistry in hot Cores with ALMA-Selected oxygen-bearing species

Y Chen, ML Van Gelder, P Nazari, CL Brogan… - Astronomy & …, 2023 - aanda.org
Context. Complex organic molecules (COMs), especially the oxygen-bearing species, have
been observed to be abundant in the gas phase toward low-mass and high-mass protostars …

A global view on star formation: The GLOSTAR Galactic plane survey-I. Overview and first results for the Galactic longitude range 28°< l< 36°

A Brunthaler, KM Menten, SA Dzib, WD Cotton… - Astronomy & …, 2021 - aanda.org
Aims. Surveys of the Milky Way at various wavelengths have changed our view of star
formation in our Galaxy considerably in recent years. In this paper we give an overview of …

Constraining the pitch angle of the galactic spiral arms in the Milky Way

JP Vallée - New Astronomy Reviews, 2017 - Elsevier
We carry out analyses of some parameters of the galactic spiral arms, in the currently
available samples. We present a catalog of the observed pitch angle for each spiral arm in …

Galactocentric variation of the gas-to-dust ratio and its relation with metallicity

A Giannetti, S Leurini, C König, JS Urquhart… - Astronomy & …, 2017 - aanda.org
Context. The assumption of a gas-to-dust mass ratio γ is a common approach to estimate the
basic properties of molecular clouds, such as total mass and column density of molecular …

The Core Population and Kinematics of a Massive Clump at Early Stages: An Atacama Large Millimeter/submillimeter Array View

E Redaelli, S Bovino, P Sanhueza, K Morii… - The Astrophysical …, 2022 - iopscience.iop.org
High-mass star formation theories make distinct predictions on the properties of the
prestellar seeds of high-mass stars. Observations of the early stages of high-mass star …

Importance of source structure on complex organics emission-II. Do disks explain lack of methanol emission from low-mass protostars?

P Nazari, B Tabone, GP Rosotti, ML van Gelder… - Astronomy & …, 2022 - aanda.org
Context. The protostellar stage is known to be the richest star formation phase in emission
from gaseous complex organic molecules. However, some protostellar systems show little or …

Testing the Larson relations in massive clumps

A Traficante, A Duarte-Cabral, D Elia… - Monthly Notices of …, 2018 - academic.oup.com
We tested the validity of the three Larson relations in a sample of 213 massive clumps
selected from the Herschel infrared Galactic Plane (Hi-GAL) survey, also using data from the …