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astro-ph2002
The Crab Nebula: 3-dimensional Modeling
S. Shibata, H. Tomatsuri, M. Shimanuki +3
We construct an axisymmetric model for the Crab Nebula. The flow dyamics is based on the model by Kennel and Coroniti (1984), but we assume that the kinetic-energy-dominant wind is…
astro-ph2002
Pulsar Wind Nebulae and Particle Acceleration in the Pulsar Magnetosphere
S. Shibata, M. Tomatsuri, M. Shimanuki +3
This paper deals with the Crab Nebula problem to suggest that particle acceleration takes place not only at the inner shock but also over a larger region in the nebula with disorde…