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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2448

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DC Field	Value	Language
dc.contributor.author	Dodson, R.	-
dc.contributor.author	Golap, K.	-
dc.contributor.author	Osborne, J.	-
dc.contributor.author	Udaya Shankar, N.	-
dc.date.accessioned	2007-05-25T09:19:20Z	-
dc.date.available	2007-05-25T09:19:20Z	-
dc.date.issued	2002	-
dc.identifier.citation	IAU Symposium, 2002, Vol.199, p299	en
dc.identifier.uri	http://hdl.handle.net/2289/2448	-
dc.description	Restricted 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.abstract	The 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.extent	114518 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2002IAUS..199..299D	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0111354	en
dc.rights	2002 Astronomical Society of the Pacific	en
dc.title	On the association of G343.1-2.3 and PSR 1706-44	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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