806 citations · 2.5k across the 42 of their papers we have counts for
42 papers
A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar
R. A. Burns, Y. Uno, N. Sakai +34
High-mass protostars (M 8 M) are thought to gain the majority of their mass via short, intense bursts of growth. This episodic accretion is thought to be faci…
OGHReS: Large-scale filaments in the outer Galaxy
D. Colombo, C. König, J. S. Urquhart +9
Filaments are a ubiquitous morphological feature of the molecular interstellar medium and are identified as sites of star formation. In recent years, more than 100 large-scale fila…
Molecular cloud catalogue from CO(1-0) data of the Forgotten Quadrant Survey
M. Benedettini, A. Traficante, L. Olmi +13
New-generation spectroscopic surveys of the Milky Way plane have been revealing the structure of the interstellar medium, allowing the simultaneous study of dense structures from s…
The Additional Representative Images for Legacy (ARI-L) project for the ALMA Science Archive
M. Massardi, F. Stoehr, G. J. Bendo +15
The Additional Representative Images for Legacy (ARI-L) project is a European Development project for ALMA Upgrade approved by the Joint ALMA Observatory (JAO) and the European Sou…
Physical conditions in the warped accretion disk of a massive star. 349 GHz ALMA observations of G023.0100.41
A. Sanna, A. Giannetti, M. Bonfand +7
Young massive stars warm up the large amount of gas and dust which condenses in their vicinity, exciting a forest of lines from different molecular species. Their line brightness i…
Establishing the evolutionary timescales of the massive star formation process through chemistry
G. Sabatini, S. Bovino, A. Giannetti +6
(Abridged) Understanding the details of the formation process of massive (i.e. M<8-10M) stars is a long-standing problem in astrophysics. [...] We present a method to deriv…