We review electrodynamics of rotating magnetized neutron stars, from the early vacuum
model to recent numerical experiments with plasma-filled magnetospheres. Significant …

Neutron stars are fascinating astrophysical objects immersed in strong gravitational and
electromagnetic fields, at the edge of our current theories. These stars manifest themselves …

Magnetospheres of many astrophysical objects can be accurately described by the low-
inertia (or" force-free") limit of MHD. We present a new numerical method for the solution of …

We describe observations of Rotating Radio Transients (RRATs) that were discovered in a
re-analysis of the Parkes Multibeam Pulsar Survey (PMPS). The sources have now been …

Accretion flows, winds and jets of compact astrophysical objects and stars are generally
described within the framework of hydrodynamical and magnetohydrodynamical (MHD) …

We investigate in detail the properties of the stationary force-free magnetosphere of an
aligned rotator assuming the last closed field line is lying in the equatorial plane at large …

In this paper we present the results of time-dependent simulations of the dipolar
axisymmetric magnetospheres of neutron stars carried out within the frameworks of both …

The interaction of a rotating star's magnetic field with a surrounding plasma disk lies at the
heart of many questions posed by neutron stars in X-ray binaries. We consider the opening …

The current state of the art in pulsar magnetosphere modelling assumes the force-free limit
of magnetospheric plasma. This limit retains only partial information about plasma velocity …

We propose that in some pulsars the magnetosphere has different states with different
geometries or/and different distributions of currents; it occasionally switches between them …