Christoph Federrath

Australian National University

Australia

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Articles (30)

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Collaborators (20)

N M Pingel

University of Wisconsin-Madison

UNITED STATES

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Philip Mocz

Princeton University

UNITED STATES

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Neco Kriel

Australian National University

AUSTRALIA

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Anna Rosen

Assistant Professor

San Diego State University

UNITED STATES

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Romain Teyssier

Princeton University

UNITED STATES

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Mark Krumholz

Professor

Australian National University

AUSTRALIA

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N M McClure-Griffiths

Australian National University

AUSTRALIA

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Roland Crocker

Australian National University

AUSTRALIA

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JOHN BALLY

Professor

University of Colorado Boulder

UNITED STATES

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David Collins

Florida State University

UNITED STATES

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Ashley Thomas Barnes

European Southern Observatory

GERMANY

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Tim Bedding

University of Sydney

AUSTRALIA

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Shantanu Basu

Professor

University of Western Ontario Faculty of Science

CANADA

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Joss Bland-Hawthorn

ARC Laureate Professor

University of Sydney

AUSTRALIA

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Freeke van de Voort

Royal Society University Research Fellow & lecturer (proleptic)

Cardiff University

UNITED KINGDOM

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Amit Seta

Australian National University

AUSTRALIA

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Ralf Stephan Klessen

Professor

Ruprecht Karls Universität Heidelberg

GERMANY

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Jeremy Sanders

Max Planck Institute for Extraterrestrial Physics

GERMANY

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Matt L Sampson

Australian National University

AUSTRALIA

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Matthew W Kunz

Princeton University

UNITED STATES

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Christoph Federrath

Research Interests

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Articles (30)

Projection-angle effects when “observing” a turbulent magnetized collapsing molecular cloud

A comparison of the turbulent dynamo in weakly-collisional and collisional plasmas: from subsonic to supersonic turbulence

Turbulence inference from CO spectral observations

Taking control of compressible modes: bulk viscosity and the turbulent dynamo

Galactic seismology: can the Gaia ‘phase spiral’ co-exist with a clumpy, turbulent interstellar medium?

Understanding gas mixing in the circumgalactic medium

Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions

On the kinematic and thermodynamic state of clouds in complex wind–multicloud environments using a friends-of-friends analysis

The spectrum of magnetized turbulence in the interstellar medium

Formation of filaments and feathers in disc galaxies: Is self-gravity enough?

Turbulent Gas-rich Disks at High Redshift: Bars and Bulges in a Radial Shear Flow

Wide-binary eccentricity distribution in young star clusters: Dependence on the binary separation and mass

Turbulence statistics of H i clouds entrained in the Milky Way’s nuclear wind

Amplification and Saturation of Turbulent Magnetic Fields in Collapsing Primordial Gas Clouds

Measuring the hot ICM velocity structure function using XMM–Newton observations

Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence

Outflows driven by direct and reprocessed radiation pressure in massive star clusters

Critical magnetic Reynolds number of the turbulent dynamo in collisionless plasmas

Growth or Decay – I: universality of the turbulent dynamo saturation

Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence

What Sets the Star Formation Rate of Molecular Clouds? The Density Distribution as a Fingerprint of Compression and Expansion Rates

A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud

Multiphase condensation in cluster haloes

Erratum: “The Link between Turbulence, Magnetic Fields, Filaments, and Star Formation in the Central Molecular Zone Cloud G0.253+0.016” (2016, ApJ, 832, 143)

Turbulence generation by shock interaction with a highly nonuniform medium

Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds

Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field

Turbulent diffusion of streaming cosmic rays in compressible, partially ionized plasma

The role of the turbulence driving mode for the initial mass function

Infrared radiation feedback does not regulate star cluster formation

Collaborators (20)

N M Pingel

Philip Mocz

Neco Kriel

Anna Rosen

Romain Teyssier

Mark Krumholz

N M McClure-Griffiths

Roland Crocker

JOHN BALLY

David Collins

Ashley Thomas Barnes

Tim Bedding

Shantanu Basu

Joss Bland-Hawthorn

Freeke van de Voort

Amit Seta

Ralf Stephan Klessen

Jeremy Sanders

Matt L Sampson

Matthew W Kunz

Make your next move.