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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2470

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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