activity
20242026
most citedDust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains

3 citations · 3 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Itô tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics

Eric R. Moseley, R. Teyssier, Tom Abel

Lagrangian tracer particles have long been used to track the history of individual gas parcels in hydrodynamical codes. Particles advected by the cell-centered velocity carry no re…

astro-ph.GA2026

The SPHINX public data release. II. Using low-ionisation absorption lines and dust attenuation to predict Lyman continuum escape

Valentin Mauerhofer, Jérémy Blaizot, Thibault Garel +11

Low-ionisation state (LIS) absorption lines, such as SiII 1526, are widely used to trace the properties of the interstellar medium (ISM) in galaxies. These lines provide crucial in…

astro-ph.GA2025

Comparing subgrid models for cosmic ray diffusion in a magnetized isolated galaxy simulation

Sarah Thiele, Romain Teyssier

Galactic cosmic rays (CRs) play a crucial role in galaxy formation and evolution by altering gas dynamics and chemistry across multiple scales. Typical numerical simulations of CR…

astro-ph.GA2025

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium

Matt L. Sampson, James R. Beattie, Romain Teyssier +5

Cosmic rays (CRs) are an integral part of the non-thermal pressure budget in the interstellar medium (ISM) and are the leading-order ionization mechanism in cold molecular clouds.…

astro-ph.GA2024★ 3 cited

Dust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains

Eric R. Moseley, Romain Teyssier

We investigate the gas-grain relative drift velocity distributions of charged astrophysical dust grains in MHD turbulence. We do this using a range of MHD-PIC simulations spanning…