Title:	The Vela pulsar, the key?
Authors:	Dodson, R. Lewis, D. Legge, D. McCulloch, P.M. Reynolds, J. McConnell, D. Deshpande, A.A.
Issue Date:	2004
Publisher:	Astronomical Society of the Pacific
Citation:	IAU Symposium, 2004, Vol.218, p193
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.
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.
URI:	http://hdl.handle.net/2289/2470
Alternative Location:	http://adsabs.harvard.edu/cgi-bin/bib_query?2004IAUS..218..193D http://arxiv.org/abs/astro-ph/0403438
Copyright:	2004 Astronomical Society of the Pacific
Appears in Collections:	Research Papers (A&A)

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