activity
20192022
most citedThe sonic scale revealed by the world's largest supersonic turbulence simulation

151 citations · 322 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202124 cited

First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud

Piyush Sharda, Shyam H. Menon, Christoph Federrath +13

Studying the driving modes of turbulence is important for characterizing the impact of turbulence in various astrophysical environments. The driving mode of turbulence is parameter…

astro-ph.GA2021

A multi-shock model for the density variance of anisotropic, highly-magnetised, supersonic turbulence

James R. Beattie, Philip Mocz, Christoph Federrath +1

Shocks form the basis of our understanding for the density and velocity statistics of supersonic turbulent flows, such as those found in the cool interstellar medium (ISM). The var…

astro-ph.GA2020151 cited

The sonic scale revealed by the world's largest supersonic turbulence simulation

Christoph Federrath, Ralf S. Klessen, Luigi Iapichino +1

Understanding the physics of turbulence is crucial for many applications, including weather, industry, and astrophysics. In the interstellar medium (ISM), supersonic turbulence pla…

astro-ph.GA202038 cited

Magnetic field fluctuations in anisotropic, supersonic turbulence

James R. Beattie, Christoph Federrath, Amit Seta

The rich structure that we observe in molecular clouds is due to the interplay between strong magnetic fields and supersonic (turbulent) velocity fluctuations. The velocity fluctua…

astro-ph.GA201931 cited

Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds

James R. Beattie, Christoph Federrath

Stars form in highly-magnetised, supersonic turbulent molecular clouds. Many of the tools and models that we use to carry out star formation studies rely upon the assumption of clo…

astro-ph.GA201926 cited

The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds

James R. Beattie, Christoph Federrath, Ralf S. Klessen +1

Supersonic turbulence is a key player in controlling the structure and star formation potential of molecular clouds (MCs). The three-dimensional (3D) turbulent Mach number, $\mathc…