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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Wisp<br />
• Variation nature: unveiled<br />
– Synchrotron instabilities<br />
– Cmpression <strong>of</strong> e/e + pair plasma (~0.15 pc)<br />
• Radio structures (VLA) similar to<br />
optical/X-ray accelerate in the same<br />
region as for the X-ray emitting<br />
population (Bietenholz et al. 2004)<br />
2
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