The Vela pulsar, the key?
| dc.creator | Dodson, Richard | |
| dc.creator | Lewis, Dion | |
| dc.creator | Legge, David | |
| dc.creator | McCulloch, Peter | |
| dc.creator | Reynolds, John | |
| dc.creator | McConnell, David | |
| dc.creator | Deshpande, Avinash | |
| dc.date | 2004-03-18 | |
| dc.date.accessioned | 2026-07-07T02:12:40Z | |
| dc.date.available | 2026-07-07T02:12:40Z | |
| dc.description | Of all pulsars known Vela has been one of the most productive in terms in understanding pulsars and their characteristics. We present the latest results derived from Australian telescopes. These include a more accurate pulsar distance, a more precise pulsar local space velocity, a new model of the spin up and the association of a radio nebula with the X-ray pulsar wind nebula. | |
| dc.description | Poster presentation at IAU 25th meeting | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0403438 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0403438 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7533 | |
| dc.subject | Astrophysics | |
| dc.title | The Vela pulsar, the key? | |
| dc.type | text |