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

362 citations · 1.5k across the 48 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA201983 cited

The Hi-GAL catalogue of dusty filamentary structures in the Galactic Plane

E. Schisano, S. Molinari, D. Elia +27

The recent data collected by {\it Herschel} have confirmed that interstellar structures with filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to b…

astro-ph.GA201910 cited

The HASHTAG project I. A Survey of CO(3-2) Emission from the Star Forming Disc of M31

Zongnan Li, Zhiyuan Li, Matthew W. L. Smith +26

We present a CO(3-2) survey of selected regions in the M31 disc as part of the JCMT large programme, HARP and SCUBA-2 High-Resolution Terahertz Andromeda Galaxy Survey (HASHTAG). T…

astro-ph.GA2019

Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloud

Julien Montillaud, Mika Juvela, Charlotte Vastel +24

We started a multi-scale analysis of G202.3+2.5, an intertwined filamentary region of Monoceros OB1. In Paper I, we examined the distributions of dense cores and protostars and fou…

astro-ph.GA2019

Multi-scale analysis of the Monoceros OB 1 star-forming region: I. The dense core population

Julien Montillaud, Mika Juvela, Charlotte Vastel +24

Current theories and models attempt to explain star formation globally, from core scales to giant molecular cloud scales. A multi-scale observational characterisation of an entire…

astro-ph.GA2019

CHIMPS: Physical properties of molecular clumps across the inner Galaxy

A. J. Rigby, T. J. T. Moore, D. J. Eden +7

The latest generation of high-angular-resolution unbiased Galactic plane surveys in molecular-gas tracers are enabling the interiors of molecular clouds to be studied across a rang…

astro-ph.GA2019

Magnetic fields in the infrared dark cloud G34.43+0.24

Archana Soam, Tie Liu, B-G Andersson +11

We present the B-fields mapped in IRDC G34.43+0.24 using 850\,m polarized dust emission observed with the POL-2 instrument at JCMT. We examine the magnetic field geometries and…