activity
20152025
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 2k across the 73 of their papers we have counts for

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Showing 2022 · astro-ph.GAShow all

14 papers · 2 filters

astro-ph.GA2022★ 26 cited

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

Tao-Chung Ching, Keping Qiu, Di Li +154

We present 850 m dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter a…

astro-ph.GA2022★ 78 cited

The Star Formation Rate of the Milky Way as seen by Herschel

D. Elia, S. Molinari, E. Schisano +23

We present a new derivation of the Milky Way's current star formation rate (SFR) based on the data of the Hi-GAL Galactic plane survey. We estimate the distribution of the SFR acro…

astro-ph.GA2022★ 18 cited

12CO (3-2) High-Resolution Survey (COHRS) of the Galactic Plane: Complete Data Release

Geumsook Park, Malcolm J. Currie, Holly S. Thomas +9

We present the full data release of 12CO (3-2) High-Resolution Survey (COHRS), which has mapped the inner Galactic plane over the range of 9.5 l 62.3$^{\circ}…

astro-ph.GA2022★ 31 cited

The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2

Jihye Hwang, Jongsoo Kim, Kate Pattle +157

We present and analyze observations of polarized dust emission at 850 m towards the central 1 pc 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obta…

astro-ph.GA2022★ 14 cited

ATLASGAL -- Star forming efficiencies and the Galactic star formation rate

M. R. A. Wells, J. S. Urquhart, T. J. T. Moore +5

The ATLASGAL survey has characterised the properties of approximately 1000 embedded HII regions and found an empirical relationship between the clump mass and bolometric luminosity…

astro-ph.GA2022★ 9 cited

Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds

Raffaele Rani, Toby J. T. Moore, David J. Eden +1

It is speculated that the high star-formation efficiency observed in spiral-arm molecular clouds is linked to the prevalence of compressive (curl-free) turbulent modes, while the s…