X-ray observations of the young pulsar wind nebula G21.5–0.9 and the evolved pulsar wind nebulae CTB 87 (G74.9+1.2) and G63.7+1.1
Pulsar wind nebulae (PWNe), nebulae harbouring a rotation-powered neutron star that was born in a supernova, provide opportunities to study highly relativistic pulsar winds and their interaction with the surrounding medium. Particularly interesting are PWNe that do not show any sign of the expected...
Main Author: | |
---|---|
Other Authors: | |
Published: |
IOP Publishing Ltd. for The American Astronomical Society
2015
|
Subjects: | |
Online Access: | http://hdl.handle.net/1993/30163 |