Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

Constraining dynamo theories of magnetic field origin by observation is indispensable but
challenging, in part because the basic quantities measured by observers and predicted by …

We discuss new methods to integrate the cosmic ray (CR) evolution equations coupled to
magnetohydrodynamics on an unstructured moving mesh, as realized in the massively …

The physics of cosmic rays (CRs) is a promising candidate for explaining the driving of
galactic winds and outflows. Recent galaxy formation simulations have demonstrated the …

In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

We study the formation of galactic outflows from supernova (SN) explosions with the moving-
mesh code AREPO in a stratified column of gas with a surface density similar to the Milky …

Most of the visible matter in the Universe is ionized, so that cosmic magnetic fields are quite
easy to generate and due to the lack of magnetic monopoles hard to destroy. Magnetic fields …

Star formation in galaxies appears to be self-regulated by energetic feedback processes.
Among the most promising agents of feedback are cosmic rays (CRs), the relativistic ion …

We review numerical methods for simulations of cosmic ray (CR) propagation on galactic
and larger scales. We present the development of algorithms designed for …

We present a study of the filamentary structure in the neutral atomic hydrogen (HI) emission
at the 21 cm wavelength toward the Galactic plane using the 16′. 2-resolution observations …