Laboratory facilities employing high pulsed currents and voltages, and called generally
“pulsed-power facilities,” allow experimenters to produce a variety of hydrodynamical …

Fully general relativistic models of astrophysical sources are in high demand, not only since
the discovery of gravitational waves emitted from merging stellar mass black holes (Abbott et …

In this review, the equations of hydrodynamics, magnetohydrodynamics, and radiation
hydrodynamics are presented, together with their corresponding nonideal source terms. I …

We study the behavior of magnetorotational turbulence in shearing box simulations with a
radial and azimuthal extent up to 10 scale heights. Maxwell and Reynolds stresses are …

Planets appear to form in environments shaped by the gas flowing through protostellar disks
to the central young stars. The flows in turn are governed by orbital angular momentum …

Recent progress in understanding the physics of magnetic reconnection is conveniently
summarized in terms of a phase diagram which organizes the essential dynamics for a wide …

We have systematically studied a large sample of the neutron star low-mass X-ray binaries
(LMXBs) monitored by the Rossi X-ray Timing Explorer (50 sources; 10000+ observations) …

The magnetorotational instability (MRI) is the most promising mechanism by which angular
momentum is efficiently transported outwards in astrophysical discs. However, its application …

The dynamo driven by the magnetorotational instability (MRI) is believed to play an
important role in the dynamics of accretion discs and may also explain the origin of the …

Convection is ubiquitous in stars and occurs under many different conditions. Here we
explore convection in main-sequence stars through two lenses: dimensionless parameters …