Physics
Scientific paper
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.
Berry Daniel L.
Luz M. G. C. D.
No associations
LandOfFree
Pulsar-Supernova Remnant Interaction: a Simple Model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Pulsar-Supernova Remnant Interaction: a Simple Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsar-Supernova Remnant Interaction: a Simple Model will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1786861