collaborators

7 papers

astro-ph.HE2026

RAMSES-MCR: A consistent multi-group treatment of cosmic rays physics in momentum-space with the RAMSES code

Nimatou-Seydi Diallo, Yohan Dubois, Alexandre Marcowith +2

Cosmic rays (CRs) are known to play a key role in many astrophysical environments: they can modify shock dynamics, influence the thermochemistry and the ionization of the interstel…

astro-ph.SR2026

Numerical Insights into Disk Accretion, Eccentricity, and Kinematics in the Class 0 phase

Adnan Ali Ahmad, Benoît Commerçon, Elliot Lynch +4

The formation and early evolution of protoplanetary disks are governed by a wide variety of physical processes during a gravitational collapse. Observations have begun probing disk…

astro-ph.IM2025

A highly accurate drag solver for multi-fluid dust and gas hydrodynamics on GPUs

L. Sewanou, G. Laibe, B. Commerçon

Exascale supercomputing unleashes the potential for simulations of astrophysical systems with unprecedented resolution. Taking full advantage of this computing power requires the d…

astro-ph.SR2025

Turn up the light: Radiative efficiency of protostars at birth

Asmita Bhandare, Adnan Ali Ahmad, Benoît Commerçon

Early stages of stellar birth comprise of a two-step process involving the formation of two hydrostatic cores. The second step of gravitational collapse sets the radiative efficien…

astro-ph.GA2025

PRODIGE VI -- Envelope to Disk with NOEMA: VI. The Missing Sulfur Problem

J. J. Miranzo-Pastor, A. Fuente, D. Navarro-Almaida +17

Determining the amount of sulfur in volatiles and refractories in the ISM remains one of the main problems in astrochemistry. The detection of HS ices, which are thought to be…

astro-ph.SR2025

Birth of magnetized low-mass protostars and circumstellar disks

Adnan Ali Ahmad, Matthias González, Patrick Hennebelle +2

Although protostars and disks are often studied separately owing to numerical and observational challenges, breakthroughs in recent years have highlighted the need to study both ob…