activity
20082026
most citedPhantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics

431 citations · 1.8k across the 39 of their papers we have counts for

collaborators
Showing 2021Show all

5 papers · 1 filter

astro-ph.GA2021★ 29 cited

The formation and early evolution of embedded star clusters in spiral galaxies

Steven Rieder, Clare Dobbs, Thomas Bending +2

We present Ekster, a new method for simulating star clusters from birth in a live galaxy simulation that combines the smoothed-particle hydrodynamics (SPH) method Phantom with the…

astro-ph.GA2021★ 36 cited

The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation and magnetic walls during the early stages of star formation

James Wurster, Matthew R. Bate, Ian A. Bonnell

Non-ideal magnetohydrodynamic (MHD) processes -- namely Ohmic resistivity, ambipolar diffusion and the Hall effect -- modify the early stages of the star formation process and the…

astro-ph.GA2021★ 16 cited

Investigating the role of magnetic fields in star formation using molecular line profiles

Charles Yin, Felix D. Priestley, James Wurster

Determining the importance of magnetic fields in star forming environments is hampered by the difficulty of accurately measuring both field strength and gas properties in molecular…

astro-ph.GA2021★ 18 cited

The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds

C. L. Dobbs, J. Wurster

We have performed Smoothed Particle Magneto-Hydrodynamics (SPMHD) calculations of colliding clouds to investigate the formation of massive stellar clusters, adopting a timestep cri…

astro-ph.SR2021★ 25 cited

Do we need non-ideal magnetohydrodynamics to model protostellar discs?

James Wurster

We investigate and discuss protostellar discs in terms of where the various non-ideal magnetohydrodynamics (MHD) processes are important. We find that the traditional picture of a…