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A Model for the Spatial Distribution of Relativistic Electrons in the Crab Nebula
Published online by Cambridge University Press: 25 May 2016
Abstract
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A model for the spatial distribution of relativistic electrons in the Crab Nebula is proposed. Particles injected in the vicinity of the pulsar propagate in a magnetic field of time-dependent but spatially constant intensity. A good description of the nebular synchrotron emission, from radio to X-ray frequencies, is obtained if particle diffusion with respect to the azimuthal field lines is taken into account.
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