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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 …
The episodic and multiscale Galactic Centre
A Bryant, A Krabbe - New Astronomy Reviews, 2021 - Elsevier
Within the central few hundred parsecs of the Milky Way, extending from longitude l=− 1° to
1.5°, lies the Central Molecular Zone of the Galactic Centre. This extraordinary region is …
1.5°, lies the Central Molecular Zone of the Galactic Centre. This extraordinary region is …
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 …
Star cluster progenitors are dynamically decoupled from their parent molecular clouds
The formation of stellar clusters dictates the pace at which galaxies evolve, and solving the
question of their formation will undoubtedly lead to a better understanding of the Universe as …
question of their formation will undoubtedly lead to a better understanding of the Universe as …
The Milky Way atlas for linear filaments
Context. Filamentary structure is important for the ISM and star formation. Galactic
distribution of filaments may regulate the star formation rate in the Milky Way. However …
distribution of filaments may regulate the star formation rate in the Milky Way. However …
The population of the galactic center filaments: position angle distribution reveals a degree-scale collimated outflow from Sgr A* along the galactic plane
We have examined the distribution of the position angle (PA) of the Galactic center filaments
with lengths L> 66''and< 66''as well as their length distribution as a function of PA. We find …
with lengths L> 66''and< 66''as well as their length distribution as a function of PA. We find …
GAUSSPY+: A fully automated Gaussian decomposition package for emission line spectra
Our understanding of the dynamics of the interstellar medium is informed by the study of the
detailed velocity structure of emission line observations. One approach to study the velocity …
detailed velocity structure of emission line observations. One approach to study the velocity …
The Multilayer Nature of Molecular Gas toward the Cygnus Region
S Zhang, Y Su, X Chen, M Fang, QZ Yan… - The Astronomical …, 2024 - iopscience.iop.org
We study the physical properties and 3D distribution of molecular clouds (MCs) toward the
Cygnus region using the MWISP CO survey and Gaia DR3 data. Based on Gaussian …
Cygnus region using the MWISP CO survey and Gaia DR3 data. Based on Gaussian …
Galactic 'Snake'IRDC G11. 11− 0.12: a site of multiple hub–filament systems and colliding filamentary clouds
To probe star formation processes, we present a multiscale and multiwavelength
investigation of the 'Snake'nebula/infrared dark cloud G11. 11− 0.12 (hereafter, G11; …
investigation of the 'Snake'nebula/infrared dark cloud G11. 11− 0.12 (hereafter, G11; …
A global view on star formation: The GLOSTAR Galactic plane survey-VIII. Formaldehyde absorption in Cygnus X
Context. Cygnus X is one of the closest and most active high-mass star-forming regions in
our Galaxy, making it one of the best laboratories for studying massive star formation. Aims …
our Galaxy, making it one of the best laboratories for studying massive star formation. Aims …