362 citations · 5.3k across the 126 of their papers we have counts for
8 papers · 2 filters
36 GHz methanol lines from nearby galaxies: maser or quasi-thermal emission?
P. Humire, C. Henkel, Y. Gong +12
Methanol (CH3OH) is one of the most abundant interstellar molecules, offering a vast number of transitions to be studied, including many maser lines. While the strongest Galactic C…
On the size of the CO-depletion radius in the IRDC G351.77-0.51
G. Sabatini, A. Giannetti, S. Bovino +5
An estimate of the degree of CO-depletion () provides information on the physical conditions occurring in the innermost and densest regions of molecular clouds. A key paramete…
ATLASGAL -- physical parameters of dust clumps associated with 6.7 GHz methanol masers
S. J. Billington, J. S. Urquhart, C. Konig +9
We have constructed the largest sample of dust-associated class II 6.7 GHz methanol masers yet obtained. New measurements from the the Methanol MultiBeam (MMB) Survey were combined…
Warm gas in protostellar outflows. II. EHV jet and outflows from OMC-2/3
A. I. Gómez-Ruiz, A. Gusdorf, S. Leurini +4
OMC-2/3 is one of the nearest embedded cluster-forming region that includes intermediate-mass protostars at early stages of evolution. A previous CO (3--2) mapping survey towards t…
Massive and low-mass protostars in massive "starless" cores
Thushara Pillai, Jens Kauffmann, Qizhou Zhang +5
The infrared dark clouds (IRDCs) G11.110.12 and G28.340.06 are two of the best-studied IRDCs in our Galaxy. These two clouds host clumps at different stages of evolution, inc…
ATLASGAL --- Molecular fingerprints of a sample of massive star forming clumps
J. S. Urquhart, C. Figura, F. Wyrowski +10
We have conducted a 3-mm molecular-line survey towards 570 high-mass star-forming clumps, using the Mopra telescope. The sample is selected from the 10,000 clumps identified by the…
A timeline for massive star-forming regions via combined observation of o-HD and ND
A. Giannetti, S. Bovino, P. Caselli +6
Context: In cold and dense gas prior to the formation of young stellar objects, heavy molecular species (including CO) are accreted onto dust grains. Under these conditions H…
ATLASGAL-selected high-mass clumps in the inner Galaxy. VII. Characterisation of mid-J CO emission
Felipe Navarete, Silvia Leurini, Andrea Giannetti +7
High-mass stars are formed within massive molecular clumps, where a large number of stars form close together. The evolution of the clumps with different masses and luminosities is…