collaborators

7 papers

astro-ph.GA2025

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.GA2025

The Evolutionary Path of Star-Forming Clumps in Hi-GAL

Ylenia Maruccia, Stefano Cavuoti, Massimo Brescia +4

Star formation (SF) studies are benefiting from the huge amount of data made available by recent large-area Galactic plane surveys conducted between 2 μm and 3 mm. Fully character…

astro-ph.GA2025

PRIMAGAL: a PRIMAger Galactic Plane Far-IR polarization survey to quantify the magnetic fields' role in the formation and evolution of large star-forming filaments

S. Molinari, J. D. Soler, V. -M. Pelkonen +8

The PRIMAger instrument on board the proposed PRIMA satellite will offer the unprecedented capability to obtain hundreds of square-degree maps in polarised emission at sub-arcminut…

astro-ph.GA2025

Star formation efficiency and scaling relations in parsec-scale cluster-forming clumps

V. Rawat, M. R. Samal, A. Zavagno +5

Numerical simulations predict that clumps (1 pc) should form stars at high efficiency to produce bound star clusters. We conducted a statistical study of 17 nearby cluster-fo…