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20112026
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 2.1k across the 55 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019★ 26 cited

The 3D structure of CO depletion in high-mass prestellar regions

S. Bovino, S. Ferrada-Chamorro, A. Lupi +3

Disentangling the different stages of the star-formation process, in particular in the high-mass regime, is a challenge in astrophysics. Chemical clocks could help alleviating this…

astro-ph.GA2019★ 30 cited

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…

astro-ph.IM2019★ 1 cited

ALMA FITS header keywords: a study from the archive User perspective

Elisabetta Liuzzo, Marcella Massardi, Kazi L. J. Rygl +7

ALMA products are stored in the Science Archive in the form of FITS images. It is a common idea that the FITS image headers should collect in their keywords all the information tha…

astro-ph.GA2019★ 34 cited

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…

astro-ph.GA2019★ 23 cited

Small-scale physical and chemical structure of diffuse and translucent molecular clouds along the line of sight to Sgr B2

V. Thiel, A. Belloche, K. M. Menten +7

The diffuse and translucent molecular clouds traced in absorption along the line of sight to strong background sources have so far been investigated mainly in the spectral domain b…

astro-ph.GA2019★ 23 cited

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…