The Evolution & Structure of Pulsar Wind Nebulae
The Evolution & Structure of Pulsar Wind Nebulae
The Evolution & Structure of Pulsar Wind Nebulae
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• Optical:<br />
Filaments<br />
– R-T instabilities as the<br />
expanding relativistic<br />
bubble sweeps up and<br />
accelerates slower<br />
moving ejecta (Hester<br />
et al. 1996)<br />
– simulation 60-75%<br />
mass concerntration<br />
(eg.,Jun 1998)<br />
2