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astro-ph2003
A Key to Pulsar Wind Bubble Morphologies: HD simulations
Eric van der Swaluw, Turlough P. Downes
We present a model of a pulsar-driven supernova remnant, by using a hydrodynamics code, which simulates the evolution of a pulsar wind nebula when the pulsar is moving at a high ve…
astro-ph2003
Particle acceleration in supernova remnants, the Bell-Lucek hypothesis and the cosmic ray "knee"
L. O'C. Drury, E. van der Swaluw, O. Carroll
Young supernova remnants are thought to be the sites where cosmic ray acceleration occurs by the mechanism of diffusive shock acceleration. The maximum energy gained in this proces…