362 citations · 2.1k across the 55 of their papers we have counts for
8 papers · 1 filter
Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA
G. Sabatini, C. Gruppioni, M. Massardi +5
The local Seyfert 2 galaxy NGC5135, thanks to its almost face-on appearance, a bulge overdensity of stars, the presence of a large-scale bar, an AGN and a Supernova Remnant, is an…
ATLASGAL-selected massive clumps in the inner Galaxy: VI. Kinetic temperature and spatial density measured with formaldehyde
X. D. Tang, C. Henkel, F. Wyrowski +11
We aim to directly determine the kinetic temperature and spatial density with formaldehyde for the 100 brightest ATLASGAL-selected clumps at 870 m representing various evo…
Galactocentric variation of the gas-to-dust ratio and its relation with metallicity
A. Giannetti, S. Leurini, C. Koenig +6
(Abridged) Context: The assumption of a gas-to-dust mass ratio (γ) is a common approach to estimate the basic properties of molecular clouds, such as total mass and column density…
Fast deuterium fractionation in magnetized and turbulent filaments
Bastian Körtgen, Stefano Bovino, Dominik R. G. Schleicher +4
Deuterium fractionation is considered as an important process to infer the chemical ages of prestellar cores in filaments. We present here the first magneto-hydrodynamical simulati…
ATLASGAL --- properties of a complete sample of Galactic clumps
J. S. Urquhart, C. Koenig, A. Giannetti +15
Abridged: ATLASGAL is an unbiased 870 micron submillimetre survey of the inner Galactic plane. It provides a large and systematic inventory of all massive, dense clumps in the Gala…
ATLASGAL-selected massive clumps in the inner Galaxy: V. Temperature structure and evolution
A. Giannetti, S. Leurini, F. Wyrowski +5
(Abridged) Aims: We aim to use the progressive heating of the gas caused by the feedback of high-mass young stellar objects (YSOs) to prove the statistical validity of the most com…