Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …

Understanding the physics of turbulence is crucial for many applications, including weather,
industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …

Context. Density and velocity fluctuations on virtually all scales observed with modern
telescopes show that molecular clouds (MCs) are turbulent. The forcing and structural …

Astrophysical gases are commonly multiphase and highly turbulent. In this work, we
investigate the survival and growth of cold gas in such a turbulent, multiphase medium using …

We study the star formation efficiency (SFE) in simulations and observations of turbulent,
magnetized, molecular clouds. We find that the probability density functions (PDFs) of the …

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 …

We present results of large-scale three-dimensional simulations of supersonic Euler
turbulence with the piecewise parabolic method and multiple grid resolutions up to 2048 3 …

We review the present theoretical and numerical understanding of magnetic field
amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond …

Nonhelical hydromagnetic forced turbulence is investigated using large scale simulations on
up to 256 processors and 1024 3 mesh points. The magnetic Prandtl number is varied …