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 …
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°
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 …
the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey:
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …
The origin of massive stars: The inertial-inflow model
We address the problem of the origin of massive stars, namely the origin, path, and
timescale of the mass flows that create them. Based on extensive numerical simulations, we …
timescale of the mass flows that create them. Based on extensive numerical simulations, we …
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 …
The dynamical evolution of molecular clouds near the Galactic Centre–I. Orbital structure and evolutionary timeline
JMD Kruijssen, JE Dale… - Monthly Notices of the …, 2015 - academic.oup.com
We recently proposed that the star-forming potential of dense molecular clouds in the
Central Molecular Zone (CMZ, ie the central few 100 pc) of the Milky Way is intimately linked …
Central Molecular Zone (CMZ, ie the central few 100 pc) of the Milky Way is intimately linked …
HCN-to-HNC intensity ratio: a new chemical thermometer for the molecular ISM
A Hacar, AD Bosman, EF Van Dishoeck - Astronomy & Astrophysics, 2020 - aanda.org
Context. The gas kinetic temperature (TK) determines the physical and chemical evolution of
the interstellar medium (ISM). However, obtaining reliable TK estimates usually requires …
the interstellar medium (ISM). However, obtaining reliable TK estimates usually requires …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores
We present dynamical properties of 294 cores embedded in twelve IRDCs observed as part
of the ASHES Survey. Protostellar cores have higher gas masses, surface densities, column …
of the ASHES Survey. Protostellar cores have higher gas masses, surface densities, column …
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 …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs
The initial conditions found in infrared dark clouds (IRDCs) provide insights on how high-
mass stars and stellar clusters form. We have conducted high-angular resolution and high …
mass stars and stellar clusters form. We have conducted high-angular resolution and high …