activity
20222026
most citedProtostellar collapse simulations in spherical geometry with dust coagulation and fragmentation

52 citations · 62 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes

Gabriel Verrier, Patrick Hennebelle, Ugo Lebreuilly +1

Interstellar grains play key roles in star and planet formation, including the coupling of the gas to the magnetic field during the protostellar collapse. These roles depend on the…

astro-ph.SR2025★ 1 cited

Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks

V. Vallucci-Goy, U. Lebreuilly, M. -M. Mac Low +1

Context: The streaming instability (SI) is a leading candidate for reaching solid densities sufficient to trigger the gravitational collapse needed for the formation of planetesima…

astro-ph.GA2025

Magnetic clumping of charged dust in the dense interstellar medium

V. Vallucci-Goy, P. Hennebelle, U. Lebreuilly +1

Context: Dust grains undergo significant growth in star-forming environments, especially in dense regions prone to gravitational collapse. Although dust is generally assumed to rep…

astro-ph.SR2024★ 9 cited

Dust evolution during the protostellar collapse: influence on the coupling between the neutral gas and the magnetic field

Valentin Vallucci-Goy, Ugo Lebreuilly, Patrick Hennebelle

The coupling between the magnetic field and the gas during the collapsing phase of star-forming cores is strongly affected by the dust size distribution, which is expected to evolv…

astro-ph.GA2022★ 52 cited

Protostellar collapse simulations in spherical geometry with dust coagulation and fragmentation

Ugo Lebreuilly, Valentin Vallucci-Goy, Vincent Guillet +2

We model the coagulation and fragmentation of dust grains during the protostellar collapse with our newly developed shark code. It solves the gas-dust hydrodynamics in a spherical…