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Diffusion in Pulsar Wind Nebulae: An Investigation using Magnetohydrodynamic and Particle Transport Models (2016)

First Author: Porth O

Attributed to: Dynamics of Relativistic Magnetized Flows. funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1604.03352

Publication URI: https://arxiv.org/abs/1604.03352

Type: Other