activity
20232025
most citedAccuracy of ALMA estimates of young disk radii and masses. Predicted observations from numerical simulations

16 citations · 22 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025★ 5 cited

The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations

Ngo-Duy Tung, Alessio Traficante, Ugo Lebreuilly +13

Context. The evolution of massive star-forming clumps that are progenitors of high-mass young stellar objects are often classified based on a variety of observational indicators ra…

astro-ph.SR2025

The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps

Ugo Lebreuilly, Alessio Traficante, Alice Nucara +14

Context. Star formation and, in particular, high-mass star formation are key astrophysical processes that are far from being fully understood. Unfortunately, progress in these fiel…

astro-ph.SR2025

The Rosetta Stone project. III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps

Alice Nucara, Alessio Traficante, Ugo Lebreuilly +23

The physical mechanisms that regulate the collapse of high-mass parsec-scale clumps and allow them to form clusters of new stars represent a crucial aspect of star formation. To in…

astro-ph.SR2024

Planet Formation and Disk Chemistry: Dust and Gas Evolution during Planet Formation

G. Perotti, L. Cacciapuoti, N. -D. Tung +3

Over the past decade, progress in observational capabilities, combined with theoretical advancements, have transformed our comprehension of the physics and chemistry during planet…

astro-ph.EP2024★ 16 cited

Accuracy of ALMA estimates of young disk radii and masses. Predicted observations from numerical simulations

Ngo-Duy Tung, Leonardo Testi, Ugo Lebreuilly +7

Protoplanetary disks, which are the natural consequence of the gravitational collapse of the dense molecular cloud cores, host the formation of the known planetary systems in our u…

astro-ph.SR2023★ 1 cited

Synthetic populations of protoplanetary disks. Impact of magnetic fields and radiative transfer

U. Lebreuilly, P. Hennebelle, T. Colman +10

Protostellar disks are the product of angular momentum conservation during the protostellar collapse. Understanding their formation is crucial because they are the birthplace of pl…