The Supernova Remnant G11.2-0.3 and its central Pulsar
Astrophysics
2009-10-28 v1
Abstract
The plerion inside the composite Supernova Remnant G11.2-0.3 appears to be dominated by the magnetic field to an extent unprecedented among well known cases. We discuss its evolution as determined by a central pulsar and the interaction with the surrounding thermal remnant, which in turn interacts with the ambient medium. We find that a plausible scenario exists, where all the observations can be reproduced with rather typical values for the parameters of the system; we also obtain the most likely period for the still undetected pulsar.
Cite
@article{arxiv.astro-ph/9604085,
title = {The Supernova Remnant G11.2-0.3 and its central Pulsar},
author = {R. Bandiera and F. Pacini and M. Salvati},
journal= {arXiv preprint arXiv:astro-ph/9604085},
year = {2009}
}
Comments
10 pages, to be published on ApJ Letters. Formatted using AASTeX