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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 2013Show all

8 papers · 1 filter

astro-ph.GA2013★ 70 cited

The Star Formation Rate of Molecular Clouds

Paolo Padoan, Christoph Federrath, Gilles Chabrier +5

We review recent advances in the analytical and numerical modeling of the star formation rate in molecular clouds and discuss the available observational constraints. We focus on m…

astro-ph.SR2013

Smoothed Particle Magnetohydrodynamics Simulations of Protostellar Jets and Turbulent Dynamos

Terrence S. Tricco, Daniel J. Price, Christoph Federrath +1

We presents results from Smoothed Particle Magnetohydrodynamics simulations of collapsing molecular cloud cores, and dynamo amplification of the magnetic field in the presence of M…

astro-ph.GA2013★ 46 cited

A measurement of the turbulence-driven density distribution in a non-star-forming molecular cloud

Adam Ginsburg, Christoph Federrath, Jeremy Darling

Molecular clouds are supersonically turbulent. This turbulence governs the initial mass function and the star formation rate. In order to understand the details of star formation,…

astro-ph.GA2013★ 84 cited

The origin of physical variations in the star formation law

Christoph Federrath

Observations of external galaxies and of local star-forming clouds in the Milky Way have suggested a variety of star formation laws, i.e., simple direct relations between the colum…

astro-ph.SR2013★ 300 cited

On the universality of supersonic turbulence

Christoph Federrath

Compressible turbulence shapes the structure of the interstellar medium of our Galaxy and likely plays an important role also during structure formation in the early Universe. The…

astro-ph.GA2013★ 67 cited

Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds

Jouni Kainulainen, Christoph Federrath, Thomas Henning

We examine the physical parameters that affect the accumulation of gas in molecular clouds to high column densities where the formation of stars takes place. In particular, we anal…