The Dynamics of the Pulsar Wind Nebula in G11.2-0.3

Details The Dynamics of the Pulsar Wind Nebula in G11.2-0.3 The Dynamics of the Pulsar Wind Nebula in G11.2-0.3

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1230r&link_type=abstract

Chandra Proposal ID #04500958

Physics

Chandra Proposal Id #04500958

Scientific paper

We propose to make a series of observations of the pulsar wind nebula in the supernova remnant G11.23-0.3 to track the motion of individual dynamic spots seen with an AO-1 observation. This will constrain the termination shock radius and help us resolve the issue of the anomalously high magnetic field inferred from broad band spectral observations. More importantly, these observations will provide insight into the dynamical properties of a "typical" PWN/SNR system. The greater integration time of the combined set will also aid in resolving the true morphology of the PWN, which remains ambiguous.

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