231 citations · 2k across the 33 of their papers we have counts for
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Clumps and triggered star formation in ionised molecular clouds
S. Walch, A. P. Whitworth, T. G. Bisbas +2
Infrared shells and bubbles are ubiquitous in the Galaxy and can generally be associated with HII regions formed around young, massive stars. In this paper, we use high-resolution…
Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
D. A. Hubber, S. A. E. G. Falle, S. P. Goodwin
We compare the results for a set of hydrodynamical tests performed with the AMR finite volume code, MG and the SPH code, SEREN. The test suite includes shock tube tests, with and w…
An improved sink particle algorithm for SPH simulations
D. A. Hubber, S. Walch, A. P. Whitworth
Numerical simulations of star formation frequently rely on the implementation of sink particles, (a) to avoid expending computational resource on the detailed internal physics of i…
A hybrid SPH/N-body method for star cluster simulations
D. A. Hubber, R. J. Allison, R. Smith +1
We present a new hybrid Smoothed Particle Hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background. By deriving t…