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Emission From Rotation-Powered Pulsars: Is It All Relative?
Alice K. Harding
Thirty-five years after the discovery of rotation-powered pulsars, we still do not understand the fundamentals of their pulsed emission at any wavelength. Even detailed pulse profi…
Polarization of pulsar radiation in the two-pole caustic model and in the outer gap model
J. Dyks, A. K. Harding, B. Rudak
We present linear polarization characteristics of pulsar radiation as predicted by two models of high-energy radiation from extended regions in the outer magnetosphere: the recentl…
Isolated Neutron Stars
V. M. Kaspi, M. S. E. Roberts, A. K. Harding
This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as we…
Physical Processes in Strong Magnetic Fields of Neutron Stars
Alice K. Harding
Neutron stars have inferred surface magnetic fields of up to 10^{14} Gauss, in the case of radio pulsars, and up to possibly 10^{15} Gauss, in the case of Soft Gamma-Ray Repeaters…
Gamma Rays From Rotation-Powered Pulsars
Alice K. Harding
The seven known gamma-ray pulsars represent a very small fraction of the more than 1000 presently known radio pulsars, yet they can give us valuable information about pulsar partic…
RXTE Observations of the Vela Pulsar: The X-ray-Optical Connection
Alice K Harding, Mark S. Strickman, Carl Gwinn +2
We report on our analysis of a 300 ks observation of the Vela pulsar with the Rossi X-Ray Timing Explorer (RXTE). The double-peaked, pulsed emission at 2 - 30 keV, which we had pre…