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20072025
most citedThe Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations

779 citations · 13.3k across the 229 of their papers we have counts for

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Showing 2011Show all

15 papers · 1 filter

astro-ph.SR2011★ 12 cited

Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification

Erik Bertram, Christoph Federrath, Robi Banerjee +1

We study the mass-to-flux ratio (M/Φ) of clumps and cores in simulations of supersonic, magnetohydrodynamical turbulence for different initial magnetic field strengths. We investig…

astro-ph.SR2011★ 90 cited

Importance of the Initial Conditions for Star Formation - III: Statistical Properties of Embedded Protostellar Clusters

Philipp Girichidis, Christoph Federrath, Richard Allison +2

We investigate the formation of protostellar clusters during the collapse of dense molecular cloud cores with a focus on the evolution of potential and kinetic energy, the degree o…

physics.flu-dyn2011★ 60 cited

Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks

Lukas Konstandin, Christoph Federrath, Ralf S. Klessen +1

We present a systematic study of the influence of different forcing types on the statistical properties of supersonic, isothermal turbulence in both the Lagrangian and Eulerian fra…

astro-ph.SR2011★ 85 cited

Importance of the Initial Conditions for Star Formation - II. Fragmentation Induced Starvation and Accretion Shielding

Philipp Girichidis, Christoph Federrath, Robi Banerjee +1

We investigate the impact of different initial conditions for the initial density profile and the initial turbulence on the formation process of protostellar clusters. We study the…

astro-ph.GA2011

MHD simulations of a supernova-driven ISM and the warm ionized medium using a positivity preserving ideal MHD scheme

Mordecai-Mark Mac Low, Alex S. Hill, M. Ryan Joung +6

We present new 3D magnetohydrodynamic (MHD) simulations of a supernova-driven, stratified interstellar medium. These simulations were run using the Waagan (2009) positivity preserv…

astro-ph.CO2011

Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization

Dominik R. G. Schleicher, Jennifer Schober, Christoph Federrath +3

We discuss the amplification of magnetic fields by the small-scale dynamo, a process that could efficiently produce strong magnetic fields in the first galaxies. In addition, we de…