Pulsar-Supernova Remnant Interaction: a Simple Model

Details Pulsar-Supernova Remnant Interaction: a Simple Model Pulsar-Supernova Remnant Interaction: a Simple Model

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..421l&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 421-424 (1997)

Physics

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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