activity
20072026
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 1.4k across the 45 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.GA2018

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.SR2018

Chasing discs around O-type (proto)stars - ALMA evidence for an SiO disc and disc wind from G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +28

We present high angular resolution 0.2 arcsec continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220G…

astro-ph.GA2018

Detection of a high-mass prestellar core candidate in W43-MM1

T. Nony, F. Louvet, F. Motte +11

Aims. To constrain the physical processes that lead to the birth of high-mass stars it is mandatory to study the very first stages of their formation. We search for high-mass analo…

astro-ph.GA2018

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

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

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…