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A new jeans resolution criterion for (M)HD simulations of self-gravitating gas: application to magnetic field amplification by gravity-driven turbulence

Implementing and comparing sink particles in AMR and SPH

Importance of the initial conditions for star formation - I. Cloud evolution and morphology

scholarly article

Importance of the initial conditions for star formation - II. Fragmentation-induced starvation and accretion shielding

artículo científico publicado en 2011

Importance of the initial conditions for star formation - III. Statistical properties of embedded protostellar clusters

artículo científico publicado en 2012

Magnetic field amplification by small-scale dynamo action: dependence on turbulence models and Reynolds and Prandtl numbers

artículo científico publicado en 2012

Magnetic field amplification during gravitational collapse - influence of turbulence, rotation and gravitational compression

artículo científico publicado en 2012

Modeling collapse and accretion in turbulent gas clouds: implementation and comparison of sink particles in AMR and SPH

scholarly article

Modeling jet and outflow feedback during star cluster formation

artículo científico publicado en 2014

The generation of strong magnetic fields during the formation of the first stars

scholarly article

The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification

scholarly article

The small-scale dynamo and non-ideal magnetohydrodynamics in primordial star formation

artículo científico publicado en 2012