914 citations · 16.2k across the 146 of their papers we have counts for
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The dependence of protoplanet migration rates on coorbital torques
Gennaro D'Angelo, Matthew R. Bate, Steve H. Lubow
We investigate the migration rates of high-mass protoplanets embedded in accretion discs via two and three-dimensional hydrodynamical simulations. The simulations follow the planet…
The Origin of the Initial Mass Function and Its Dependence on the Mean Jeans Mass in Molecular Clouds
Matthew R. Bate, Ian A. Bonnell
We investigate the dependence of stellar properties on the mean thermal Jeans mass in molecular clouds. We compare the results from the two largest hydrodynamical simulations of st…
Smoothed particle hydrodynamics with radiative transfer in the flux-limited diffusion approximation
Stuart C. Whitehouse, Matthew R. Bate
We describe the implementation and testing of a smoothed particle hydrodynamics (SPH) code that solves the equations of radiation hydrodynamics in the flux-limited diffusion (FLD)…
Synthetic infrared images and spectral energy distributions of a young low-mass stellar cluster
Ryuichi Kurosawa, Tim J. Harries, Matthew R. Bate +1
We present three-dimensional Monte Carlo radiative transfer models of a very young (<10^5 years old) low mass (50 Msun) stellar cluster containing 23 stars and 27 brown dwarfs. The…
On the properties of young multiple stars
E. J. Delgado-Donate, C. J. Clarke, M. R. Bate +1
Abridged/ We present numerical results on the properties of young binary and multiple stellar systems. Our analysis is based on a series of SPH + Nbody simulations of the fragmenta…
Massive star formation: Nurture, not nature
I. A. Bonnell, S. G. Vine, M. R. Bate
We investigate the physical processes which lead to the formation of massive stars. Using a numerical simulation of the formation of a stellar cluster from a turbulent molecular cl…