Gas-rich dwarf galaxies located outside the virial radius of their host are relatively pristine
systems and have ultralow gas cooling rates. This makes them very sensitive to heat …

Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM).
We present the first example of a direct interaction between a magnetic filament, a radio jet …

Phenomenological models of cosmic ray (CR) transport in the Milky Way can reproduce a
wide range of observations assuming that CRs scatter off of magnetic-field fluctuations with …

The discovery of diffuse radio emission in galaxy clusters proved the existence of energetic
cosmic-ray electrons and cosmic magnetic fields on Mpc-scales in the Universe …

Particle transport through localized interactions with sharp magnetic field bends in MHD
turbulence Page 1 J. Plasma Phys. (2023), vol. 89, 175890501 © The Author(s), 2023 …

Owing to the complexity of turbulent magnetic fields, modelling the diffusion of cosmic rays is
challenging. Based on the current understanding of anisotropic magnetohydrodynamic …

We study the streaming instability of GeV− 100 GeV cosmic rays (CRs) and its dam** in
the turbulent interstellar medium (ISM). We find that the dam** of streaming instability is …

Cosmic rays (CRs) play a pivotal role in sha** the thermal and dynamical properties of
astrophysical environments, such as galaxies and galaxy clusters. Recent observations …

In a weakly compressible high-β medium, pitch-angle scattering and the associated
scattering acceleration of cosmic rays (CRs) by anisotropic Alfvén and slow modes of …

Magnetic fields play an important role in the formation and evolution of a galaxy, but it is
challenging to measure them by observation. Here, we study the Seyfert galaxy NGC 3627's …