iv : a st ro - p h / 02 06 50 2 v 2 1 6 O ct 2 00 2 General Relativistic Electromagnetism and Particle Acceleration in Pulsar Polar Cap

ar X iv : a st ro - p h / 06 10 08 7 v 1 3 O ct 2 00 6 Jets and Disk - Winds from Pulsar Magnetospheres

We discuss axisymmetric force-free pulsar magnetospheres with magnetically collimated jets and a disk-wind obtained by numerical solution of the pulsar equation. This solution represents an alternative to the quasi-spherical wind solutions where a major part of the current flow is in a current sheet which is unstable to magnetic field annihilation.

ar X iv : a st ro - p h / 06 10 24 6 v 1 9 O ct 2 00 6 Special Features of Galactic Dynamics

ar X iv : a st ro - p h / 02 04 12 2 v 1 8 A pr 2 00 2 The Radio - Loud Plasma in Pulsars

The pulsar magnetosphere contains a strongly magnetized, relativistic plasma. We need to understand the physics of that plasma if we want to connect the data to the models. Our group in Socorro is mixing theory and observations in order to study the radio-loud pulsar plasma. In this paper we report on several aspects of our current work.

ar X iv : a st ro - p h / 00 10 30 1 v 1 1 6 O ct 2 00 0 1 MODEL SPECTRA OF ROTATION POWERED PULSARS IN THE INTEGRAL RANGE

The energy range of IBIS is a promising ground for testing mutual relations of distinct components expected in the spectra of high-energy radiation from rotation powered pulsars. According to some polar-cap models two such components-due to curvature and synchrotron emission-may contribute comparable amounts of power between 15 keV and 10 MeV (Rudak & Dyks, 1999). Zhang & Harding (2000) argued ...

ar X iv : a st ro - p h / 00 10 30 1 v 2 1 8 O ct 2 00 0 1 MODEL SPECTRA OF ROTATION POWERED PULSARS IN THE INTEGRAL RANGE

The energy range of IBIS is a promising ground for testing mutual relations of distinct components expected in the spectra of high-energy radiation from rotation powered pulsars. According to some polar-cap models two such components-due to curvature and synchrotron emission-may contribute comparable amounts of power between 15 keV and 10 MeV (Rudak & Dyks, 1999). Zhang & Harding (2000) argued ...