Interstellar water chemistry: from laboratory to observations
Water is a fundamental molecule in the universe. On Earth, water exists in all three phases:
gas, liquid, and solid (ice). Liquid water facilitates many chemical reactions as a solvent …
gas, liquid, and solid (ice). Liquid water facilitates many chemical reactions as a solvent …
The external photoevaporation of planet-forming discs
AJ Winter, TJ Haworth - The European Physical Journal Plus, 2022 - Springer
Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
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 …
870 μm submillimetre survey of the inner Galactic plane (| ℓ|< 60° with| b|< 1 5). It is the …
Massive star formation
JC Tan, MT Beltrán, P Caselli, F Fontani… - … and Planets VI, 2014 - books.google.com
The enormous radiative and mechanical luminosities of massive stars impact a vast range of
scales and processes, from the reionization of the universe, to the evolution of galaxies, to …
scales and processes, from the reionization of the universe, to the evolution of galaxies, to …
SILCC VI–Multiphase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionizing radiation, and cosmic rays
TE Rathjen, T Naab, P Girichidis… - Monthly Notices of …, 2021 - academic.oup.com
We present simulations of the multiphase interstellar medium (ISM) at solar neighbourhood
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
The red MSX source survey: The massive young stellar population of our galaxy
SL Lumsden, MG Hoare, JS Urquhart… - The Astrophysical …, 2013 - iopscience.iop.org
We present the Red MSX Source survey, the largest statistically selected catalog of young
massive protostars and H ii regions to date. We outline the construction of the catalog using …
massive protostars and H ii regions to date. We outline the construction of the catalog using …
The Hi-GAL compact source catalogue–II. The 360° catalogue of clump physical properties
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 …
between 70 and 500 m. This release not only completes the analogous catalogue previously …
ATLASGAL–towards a complete sample of massive star forming clumps
JS Urquhart, TJT Moore, T Csengeri… - Monthly Notices of …, 2014 - academic.oup.com
By matching infrared-selected, massive young stellar objects (MYSOs) and compact H ii
regions in the Red MSX Source survey to massive clumps found in the submillimetre …
regions in the Red MSX Source survey to massive clumps found in the submillimetre …
ATLASGAL–evolutionary trends in high-mass star formation
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 …
has been used to identify∼ 10 000 dense molecular clumps. Dedicated follow-up …
N-bearing complex organics toward high-mass protostars-Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range
P Nazari, JD Meijerhof, ML van Gelder… - Astronomy & …, 2022 - aanda.org
Context. Complex organic species are known to be abundant toward low-and high-mass
protostars. No statistical study of these species toward a large sample of high-mass …
protostars. No statistical study of these species toward a large sample of high-mass …