activity
20042026
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 5.3k across the 126 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

10 papers · 2 filters

astro-ph.GA2017★ 47 cited

ATLASGAL-selected massive clumps in the inner Galaxy: VI. Kinetic temperature and spatial density measured with formaldehyde

X. D. Tang, C. Henkel, F. Wyrowski +11

We aim to directly determine the kinetic temperature and spatial density with formaldehyde for the 100 brightest ATLASGAL-selected clumps at 870 m representing various evo…

astro-ph.GA2017★ 83 cited

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

A. Giannetti, S. Leurini, C. Koenig +6

(Abridged) 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…

astro-ph.GA2017★ 18 cited

Fast deuterium fractionation in magnetized and turbulent filaments

Bastian Körtgen, Stefano Bovino, Dominik R. G. Schleicher +4

Deuterium fractionation is considered as an important process to infer the chemical ages of prestellar cores in filaments. We present here the first magneto-hydrodynamical simulati…

astro-ph.GA2017★ 362 cited

ATLASGAL --- properties of a complete sample of Galactic clumps

J. S. Urquhart, C. Koenig, A. Giannetti +15

Abridged: ATLASGAL is an unbiased 870 micron submillimetre survey of the inner Galactic plane. It provides a large and systematic inventory of all massive, dense clumps in the Gala…

astro-ph.GA2017★ 22 cited

Nature of shocks revealed by SOFIA OI observations in the Cepheus E protostellar outflow

A. Gusdorf, S. Anderl, B. Lefloch +12

Protostellar jets and outflows are key features of the star-formation process, and primary processes of the feedback of young stars on the interstellar medium. Understanding the un…

astro-ph.GA2017★ 6 cited

Distribution of water in the G327.3-0.6 massive star-forming region

S. Leurini, F. Herpin, F. van der Tak +3

We aim at characterizing the large-scale distribution of H2O in G327.3-0.6, a massive star-forming region made of individual objects in different evolutionary phases. We investigat…

astro-ph.GA2017★ 86 cited

ATLASGAL-selected massive clumps in the inner Galaxy: V. Temperature structure and evolution

A. Giannetti, S. Leurini, F. Wyrowski +5

(Abridged) Aims: We aim to use the progressive heating of the gas caused by the feedback of high-mass young stellar objects (YSOs) to prove the statistical validity of the most com…

astro-ph.GA2017★ 86 cited

ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps

T. Csengeri, S. Bontemps, F. Wyrowski +18

The early evolution of massive cluster progenitors is poorly understood. We investigate the fragmentation properties from 0.3 pc to 0.06 pc scales of a homogenous sample of infrare…

astro-ph.GA2017★ 128 cited

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

F. Schuller, T. Csengeri, J. S. Urquhart +41

The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. We have carried out…

astro-ph.GA2017★ 9 cited

The shocked gas of the BHR71 outflow observed by Herschel: indirect evidence for an atomic jet

M. Benedettini, A. Gusdorf, B. Nisini +7

In the BHR71 region, two low-mass protostars drive two distinguishable outflows. They constitute an ideal laboratory to investigate the effects of shock chemistry and the mechanism…