757 citations · 12.6k across the 181 of their papers we have counts for
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Algorithmic comparisons of decaying, isothermal, supersonic turbulence
S. Kitsionas, C. Federrath, R. Klessen +10
Contradicting results have been reported in the literature with respect to the performance of the numerical techniques employed for the study of supersonic turbulence. We aim at ch…
Magnetic fields in star formation: from galaxies to stars
Daniel J. Price, Matthew R. Bate, Clare L. Dobbs
Magnetic fields are important at every scale in the star formation process: from the dynamics of the ISM in galaxies, to the collapse of turbulent molecular clouds to form stars an…
3D meshfree magnetohydrodynamics
S. Rosswog, D. J. Price
We describe a new method to include magnetic fields into smooth particle hydrodynamics. The derivation of the self-gravitating hydrodynamics equations from a variational principle…
The effect of magnetic fields on star cluster formation
Daniel Price, Matthew Bate
We examine the effect of magnetic fields on star cluster formation by performing simulations following the self-gravitating collapse of a turbulent molecular cloud to form stars in…
Magnetic fields and the dynamics of spiral galaxies
C. L. Dobbs, D. J. Price
We investigate the dynamics of magnetic fields in spiral galaxies by performing 3D MHD simulations of galactic discs subject to a spiral potential. Recent hydrodynamic simulations…
SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
Daniel J. Price
This paper presents SPLASH, a publicly available interactive visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations. Visualisation of SPH data is more complicated…