activity
20052020
most citedDispersal of molecular clouds by ionising radiation

231 citations · 2k across the 33 of their papers we have counts for

collaborators

32 papers

astro-ph.IM2020★ 3 cited

Gadget3 on GPUs with OpenACC

Antonio Ragagnin, Klaus Dolag, Mathias Wagner +5

We present preliminary results of a GPU porting of all main Gadget3 modules (gravity computation, SPH density computation, SPH hydrodynamic force, and thermal conduction) using Ope…

astro-ph.IM2019★ 9 cited

WVTICs -- SPH initial conditions for everyone

Alexander Arth, Julius Donnert, Ulrich Steinwandel +5

We present a novel and fast application to generate glass-like initial conditions for Lagrangian hydrodynamic schemes (e.g. Smoothed Particle Hydrodynamics (SPH)) following arbitra…

astro-ph.IM2017★ 52 cited

GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids

David A. Hubber, Giovanni P. Rosotti, Richard A. Booth

GANDALF is a new hydrodynamics and N-body dynamics code designed for investigating planet formation, star formation and star cluster problems. GANDALF is written in C++, parallelis…

astro-ph.GA2017★ 113 cited

Filamentary fragmentation in a turbulent medium

S. D. Clarke, A. P. Whitworth, A. Duarte-Cabral +1

We present the results of smoothed particle hydrodynamic simulations investigating the evolution and fragmentation of filaments that are accreting from a turbulent medium. We show…

astro-ph.EP2016★ 3 cited

Discs in misaligned binary systems

Krisada Rawiraswattana, David A. Hubber, Simon P. Goodwin

We perform SPH simulations to study precession and changes in alignment between the circumprimary disc and the binary orbit in misaligned binary systems. We find that the precessio…

astro-ph.GA2016★ 67 cited

Perturbation growth in accreting filaments

Seamus D. Clarke, Anthony P. Whitworth, David A. Hubber

We use smoothed particle hydrodynamic simulations to investigate the growth of perturbations in infinitely long, initially sub-critical but accreting filaments. The growth of these…