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

R. Bandiera·F. Pacini·M. Salvati
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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.

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R. Bandiera, F. Pacini, M. Salvati. 1996-04-16. The Supernova Remnant G11.2-0.3 and its central Pulsar. https://doi.org/10.1086/310123

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