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On the association of G343.1-2.3 and PSR 1706-44

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dc.contributor.authorDodson, R
dc.contributor.authorGolap, K
dc.contributor.authorOsborne, J
dc.contributor.authorShankar, N Udaya
dc.date.accessioned2007-05-25T09:19:20Z
dc.date.available2007-05-25T09:19:20Z
dc.date.issued2002
dc.descriptionRestricted Access. An open-access version is available at the alternative locations. The Universe at Low Radio Frequencies, Proceedings of IAU Symposium 199, held 30 Nov - 4 Dec 1999, Pune, India. Eds. A. Pramesh Rao, G. Swarup, and Gopal-Krishna, 2002.en
dc.description.abstractThe observations of the supernova remnant G343.1-2.3 with the Mauritius Radio Telescope, the Australia Compact Array, and the Hobart Single dish are presented. With these more sensitive measurements the association with the pulsar PSR1706-44 becomes much more likely. The major points from the observations are presented.en
dc.format.extent114518 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationIAU Symposium, 2002, Vol.199, p299en
dc.identifier.urihttp://hdl.handle.net/2289/2448
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2002IAUS..199..299Den
dc.relation.urihttp://arxiv.org/abs/astro-ph/0111354en
dc.rights2002 Astronomical Society of the Pacificen
dc.titleOn the association of G343.1-2.3 and PSR 1706-44en
dc.typeArticleen

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