activity
20062026
most citedATLASGAL - Compact source catalogue: 330 < l < 21 degrees

278 citations · 2.3k across the 42 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018★ 14 cited

Characterising the high-mass star forming filament G351.776--0.527 with Herschel and APEX dust continuum and gas observations

S. Leurini, E. Schisano, T. Pillai +13

G351.776-0.527 is among the most massive, closest, and youngest filaments in the inner Galactic plane and therefore it is an ideal laboratory to study the kinematics of dense gas a…

astro-ph.GA2018★ 28 cited

Feedback in W49A diagnosed with radio recombination lines and models

M. R. Rugel, D. Rahner, H. Beuther +20

We present images of radio recombination lines (RRLs) at wavelengths around 17 cm from the star-forming region W49A to determine the kinematics of ionized gas in the THOR survey (T…

astro-ph.GA2018★ 46 cited

SEDIGISM: The kinematics of ATLASGAL filaments

M. Mattern, J. Kauffmann, T. Csengeri +13

Analysing the kinematics of filamentary molecular clouds is a crucial step towards understanding their role in the star formation process. Therefore, we study the kinematics of 283…

astro-ph.GA2018★ 51 cited

Core fragmentation and Toomre stability analysis of W3(H2O): A case study of the IRAM NOEMA large program CORE

A. Ahmadi, H. Beuther, J. C. Mottram +30

The fragmentation mode of high-mass molecular clumps and the properties of the central rotating structures surrounding the most luminous objects have yet to be comprehensively char…

astro-ph.GA2018★ 32 cited

The role of spiral arms in Milky Way star formation

S. E. Ragan, T. J. T. Moore, D. J. Eden +4

What role does Galactic structure play in star formation? We have used the Herschel Hi-GAL compact-clump catalogue to examine trends in evolutionary stage over large spatial scales…

astro-ph.GA2018★ 34 cited

Fragmentation and disk formation during high-mass star formation: The IRAM NOEMA (Northern Extended Millimeter Array) large program CORE

H. Beuther, J. C. Mottram, A. Ahmadi +30

Aims: We aim to understand the fragmentation as well as the disk formation, outflow generation and chemical processes during high-mass star formation on spatial scales of individua…