Christoph Federrath
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Galaxies: Formation, Evolution, Phenomena · Solar and Space Plasma Dynamics
0000-0002-0706-2306
About
Christoph Federrath is a professor, faculty member, and associate director at the Research School of Astronomy and Astrophysics of the Australian National University. He previously was an Australian Research Council Future Fellow, Stromlo Fellow, and held postdoctoral fellowships at the Monash Centre for Astrophysics in Melbourne, the Ecole Normale Superieure de Lyon, and the Institute for Theoretical Astrophysics in Heidelberg. He studied physics at the University of Wuerzburg from 2001 to 2007 and received a Ph.D. (Dr. rer. nat.) from the University of Heidelberg in 2010.
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Publications (313)
- Computational advances and challenges in simulations of turbulence and star formation Save
- The impact of the turbulent Mach number on star formation and the initial mass function Save
- From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data Save
- ALMA Central Molecular Zone Exploration Survey (ACES) – VI. ALMA large program reveals a highly filamentary Central Molecular Zone Save
- Transition to dilatation-dominated isothermal compressible turbulence Save
- Correction to: 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 Save
- Conservation of magnetic-helicity fluctuations due to spatial decorrelation of fluxes in decaying MHD turbulence Save
- The statistics and structure of dissipation in subsonic and supersonic turbulence Save
- The turbulence driving mode in NGC7793 and NGC1313 Save
- Turbulence driving in a star-forming Milky-Way-type galaxy Save
- So Long Kolmogorov: The Forward and Backward Turbulence Cascades in a Supernovae-driven, Multiphase Interstellar Medium Save
- Mitigating numerical dissipation in simulations of subsonic turbulent flows Save
- Stellar spin in young star clusters: comparison between simulations and observations Save
- Turbulence inference from CO spectral observations Save
- Study of H i Turbulence in the SMC Using Multipoint Structure Functions Save
- Turbulent Gas-rich Disks at High Redshift: Origin of Thick Stellar Disks Through 3D “Baryon Sloshing” Save
- Statistical properties of compressible isothermal turbulence from sub- to supersonic conditions Save
- A comparison of the turbulent dynamo in weakly collisional and collisional plasmas: from subsonic to supersonic turbulence Save
- Taking control of compressible modes: bulk viscosity and the turbulent dynamo Save
- Galactic seismology: can the Gaia ‘phase spiral’ co-exist with a clumpy, turbulent interstellar medium? Save