Neutron stars are natural physical laboratories allowing us to study a plethora of
phenomena in extreme conditions. In particular, these compact objects can have very strong …

We review the state of the art of three dimensional numerical simulations of solar and stellar
dynamos. We summarize fundamental constraints of numerical modelling and the …

Abstract We present the Australian Square Kilometre Array Pathfinder localization and follow-
up observations of the host galaxy of the repeating fast radio burst (FRB) source, FRB …

We present results of three-dimensional (3D), radiation-magnetohydrodynamics (MHD)
simulations of core-collapse supernovae in full general relativity (GR) with spectral neutrino …

We explore the influence of non-axisymmetric modes on the dynamics of the collapsed core
of rotating, magnetized high-mass stars in three-dimensional simulations of a rapidly rotating …

The gravitational collapse of rapidly rotating massive stars can lead to the onset of the low
T/| W| instability within the central proto-neutron star (PNS), which leaves strong signatures …

Long-term neutrino-radiation resistive-magnetohydrodynamics simulations in full general
relativity are performed for a system composed of a massive neutron star and a torus formed …

We present a first 3D magnetohydrodynamic (MHD) simulation of oxygen, neon, and carbon
shell burning in a rapidly rotating core-collapse supernova progenitor. We also run a purely …

We assess the variance of the post-collapse evolution remnants of compact, massive, low-
metallicity stars, under small changes in the degrees of rotation and magnetic field of …

Initial distributions of pulsar periods and magnetic fields are essential components of
multiple modern astrophysical models. Not enough work has been done to properly …