The Vela pulsar, the key?
| dc.contributor.author | Dodson, R | |
| dc.contributor.author | Lewis, D | |
| dc.contributor.author | Legge, D | |
| dc.contributor.author | McCulloch, P M | |
| dc.contributor.author | Reynolds, J | |
| dc.contributor.author | McConnell, D | |
| dc.contributor.author | Deshpande, A A | |
| dc.date.accessioned | 2007-05-25T09:42:20Z | |
| dc.date.available | 2007-05-25T09:42:20Z | |
| dc.date.issued | 2004 | |
| dc.description | Restricted Access. Young Neutron Stars and Their Environments, IAU Symposium no. 218, held as part of the IAU General Assembly, 14-17 July, 2003 in Sydney, Australia. Edited by Fernando Camilo and Bryan M. Gaensler. San Francisco, CA: Astronomical Society of the Pacific, 2004. | en |
| dc.description.abstract | 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 spin-up at a glitch, and the association of a radio nebula with the X-ray pulsar wind nebula. | en |
| dc.format.extent | 98685 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | IAU Symposium, 2004, Vol.218, p193 | en |
| dc.identifier.uri | http://hdl.handle.net/2289/2470 | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of the Pacific | en |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?2004IAUS..218..193D | en |
| dc.relation.uri | http://arxiv.org/abs/astro-ph/0403438 | en |
| dc.rights | 2004 Astronomical Society of the Pacific | en |
| dc.title | The Vela pulsar, the key? | en |
| dc.type | Article | en |