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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Filaments<br />
• X-ray filaments <strong>of</strong> 3C58: associated with radio,<br />
not with optical<br />
different mechanism<br />
-magnetic loops torn<br />
from the toroial field<br />
by kink instabilities<br />
3