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 2021 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2021★ 25 cited

The evolution of temperature and density structures of OB cluster-forming molecular clumps

Yuxin Lin, Friedrich Wyrowski, Hauyu Baobab Liu +4

OB star clusters originate from parsec-scale massive molecular clumps. We aim to understand the evolution of temperature and density structures on the intermediate-scale ($\lesssim…

astro-ph.GA2021★ 19 cited

OGHReS: Large-scale filaments in the outer Galaxy

D. Colombo, C. König, J. S. Urquhart +9

Filaments are a ubiquitous morphological feature of the molecular interstellar medium and are identified as sites of star formation. In recent years, more than 100 large-scale fila…

astro-ph.GA2021★ 17 cited

Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3

S. Suri, H. Beuther, C. Gieser +29

Increasing evidence suggests that, similar to their low-mass counterparts, high-mass stars form through a disk-mediated accretion process. At the same time, formation of high-mass…

astro-ph.GA2021★ 39 cited

Establishing the evolutionary timescales of the massive star formation process through chemistry

G. Sabatini, S. Bovino, A. Giannetti +6

(Abridged) Understanding the details of the formation process of massive (i.e. M<8-10M) stars is a long-standing problem in astrophysics. [...] We present a method to deriv…

astro-ph.GA2021★ 7 cited

The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"

C. Gieser, H. Beuther, D. Semenov +30

We use sub-arcsecond resolution (0.4) observations with NOEMA at 1.37 mm to study the dust emission and molecular gas of 18 high-mass star-forming regions. We combine the…

astro-ph.GA2021★ 28 cited

Multi-scale view of star formation in IRAS 21078+5211: From clump fragmentation to disk wind

L. Moscadelli, H. Beuther, A. Ahmadi +23

In the massive star-forming region IRAS 21078+5211, a highly fragmented cluster (0.1~pc in size) of molecular cores is observed, located at the density peak of an elongated (1~pc i…

astro-ph.GA2021★ 174 cited

Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy

E. F. van Dishoeck, L. E. Kristensen, the WISH team

(abridged) Data and results from the WISH key program are summarized, designed to provide a legacy data set to address its physics and chemistry. WISH targeted ~80 sources along th…