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20122026
most citedThe SEDIGISM survey: Molecular clouds in the inner Galaxy

67 citations · 614 across the 22 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 42 cited

GASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud

N. M. Pingel, J. Dempsey, N. M. McClure-Griffiths +53

We present the most sensitive and detailed view of the neutral hydrogen (HI) emission associated with the Small Magellanic Cloud (SMC), through the combination of data from the Aus…

astro-ph.GA2021★ 30 cited

The SEDIGISM survey: a search for molecular outflows

A. Y. Yang, J. S. Urquhart, F. Wyrowski +19

Context. The formation processes of massive stars are still unclear but a picture is emerging involving accretion disks and molecular outflows in what appears to be a scaled-up ver…

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★ 24 cited

The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way

D. Colombo, A. Duarte-Cabral, A. R. Pettitt +23

The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of…

astro-ph.GA2021★ 22 cited

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde IV. The ALMA view of N113 and N159W in the LMC

X. D. Tang, C. Henkel, K. M. Menten +25

We mapped the kinetic temperature structure of two massive star-forming regions, N113 and N159W, in the Large Magellanic Cloud (LMC). We have used 1\hbox{$\,.\!\!^{\prime\pri…

astro-ph.GA2021

The MACH HI absorption survey I: Physical conditions of cold atomic gas outside of the Galactic plane

Claire E. Murray, Snežana Stanimirović, Carl Heiles +5

Tracing the transition between the diffuse atomic interstellar medium (ISM) and cold, dense gas is crucial for deciphering the star formation cycle in galaxies. Here we present MAC…