1. RRI Digital Repository
  2. 04. Astronomy and Astrophysics
  3. Research Papers (A&A)
Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2470
Full metadata record
DC FieldValueLanguage
dc.contributor.authorDodson, R.-
dc.contributor.authorLewis, D.-
dc.contributor.authorLegge, D.-
dc.contributor.authorMcCulloch, P.M.-
dc.contributor.authorReynolds, J.-
dc.contributor.authorMcConnell, D.-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2007-05-25T09:42:20Z-
dc.date.available2007-05-25T09:42:20Z-
dc.date.issued2004-
dc.identifier.citationIAU Symposium, 2004, Vol.218, p193en
dc.identifier.urihttp://hdl.handle.net/2289/2470-
dc.descriptionRestricted 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.abstractOf 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.extent98685 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2004IAUS..218..193Den
dc.relation.urihttp://arxiv.org/abs/astro-ph/0403438en
dc.rights2004 Astronomical Society of the Pacificen
dc.titleThe Vela pulsar, the key?en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2004 IAU SYM V218 p193.pdf
  Restricted Access		Restricted Access96.37 kBAdobe PDFView/Open Request a copy
Show simple item record


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.