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Stellar, Brown Dwarf, and Multiple Star Properties from Hydrodynamical Simulations of Star Cluster Formation
Matthew Bate
We report the statistical properties of stars, brown dwarfs and multiple systems obtained from the largest hydrodynamical simulation of star cluster formation to date that resolves…
Gas accretion onto planetary cores: three-dimensional self-gravitating radiation hydrodynamical calculations
Ben A. Ayliffe, Matthew R. Bate
We present results from three-dimensional, self-gravitating radiation hydrodynamical models of gas accretion by planetary cores. In some cases, the accretion flow is resolved down…
The Importance of Radiative Feedback for the Stellar Initial Mass Function
Matthew R. Bate
We investigate the effect of radiative feedback on the star formation process using radiation hydrodynamical simulations. We repeat the previous hydrodynamical star cluster formati…
Gravitational fragmentation and the formation of brown dwarfs in stellar clusters
Ian A. Bonnell, Paul C. Clark, Matthew R. Bate
We investigate the formation of brown dwarfs and very low-mass stars through the gravitational fragmentation of infalling gas into stellar clusters. The gravitational potential of…
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…
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…