Pulsar-Supernova Remnant Interaction: a Simple Model

Physics

Scientific paper

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Scientific paper

A model for the expansion of the ejecta following a supernova explosion is presented. If a pulsar remains at the site of the explosion, it emits magnetodipole radiation which is trapped inside the ejecta and contributes to its expansion through radiation pressure. If rotational effects are also included, outbursts of gas may occur at the poles of the remnant, possibly leading to a barrel-shaped supernova remnant.

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