The Supernova Remnant G11.2-0.3 and its central Pulsar

Details The Supernova Remnant G11.2-0.3 and its central Pulsar The Supernova Remnant G11.2-0.3 and its central Pulsar

1996-04-16

arxiv.org/abs/astro-ph/9604085v1

Astronomy and Astrophysics

Astrophysics

10 pages, to be published on ApJ Letters. Formatted using AASTeX

Scientific paper

10.1086/310123

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.

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