362 citations · 2.1k across the 55 of their papers we have counts for
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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…
Synthetic observations of HD towards high-mass starless cores
Joaquin. Zamponi F., Dominik R. G. Schleicher, Stefano Bovino +3
Young massive stars are usually found embedded in dense and massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteratio…
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…
ALMACAL IV: A catalogue of ALMA calibrator continuum observations
M. Bonato, E. Liuzzo, A. Giannetti +12
We present a catalogue of ALMA flux density measurements of 754 calibrators observed between August 2012 and September 2017, for a total of 16,263 observations in different bands a…
The fragmentation properties of massive protocluster gas clumps: an ALMA study
F. Fontani, B. Commerçon, A. Giannetti +5
Fragmentation of massive dense molecular clouds is the starting point in the formation of rich clusters and massive stars. Theory and numerical simulations indicate that the popula…