Vela Pulsar
From Wikipedia, the free encyclopedia
The Vela Pulsar is a radio, optical, X-ray and gamma-emitting pulsar associated with Vela Supernova Remnant, in the constellation of Vela. The association of the Vela pulsar with the Vela Supernova Remnant, made by astronomers at the University of Sydney in 1968,[1] was direct observational proof that supernovae form neutron stars
[edit] External links
- Starquake noted http://www.hartrao.ac.za/news/040707vela/index.html
- Chandra image http://chandra.harvard.edu/photo/2000/vela/index.html
- Chandra images pronounced jet http://chandra.harvard.edu/photo/2003/vela_pulsar/index.html
