The Vela pulsar wind nebula at 6 cm

Lewis, D.; Dodson, R.; McConnell, D.; Deshpande, A.A.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2669

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DC Field	Value	Language
dc.contributor.author	Lewis, D.	-
dc.contributor.author	Dodson, R.	-
dc.contributor.author	McConnell, D.	-
dc.contributor.author	Deshpande, A.A.	-
dc.date.accessioned	2007-06-11T06:32:55Z	-
dc.date.available	2007-06-11T06:32:55Z	-
dc.date.issued	2002	-
dc.identifier.citation	ASP Conference Series, 2002, Vol.271, p191	en
dc.identifier.uri	http://hdl.handle.net/2289/2669	-
dc.description	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations). Neutron Stars in Supernova Remnants, ASP Conference Series, Vol. 271, held in Boston, MA, USA, 14-17 August 2001. Eds. Patrick O. Slane and Bryan M. Gaensler. San Francisco: ASP, 2002.	en
dc.description.abstract	Observations using the Australia Telescope Compact Array at a wavelength of 6 cm have uncovered the radio counterpart to the compact X-ray neb ula surrounding the Vela pulsar. Two lobes were found oriented about the spin axis of the pulsar; starting at the edge of X-ray emission, they extend to three times the size. The northern lobe has a bright, defined edge and an integrated flux of 0.14 Jy, while the southern lobe of 0.12 Jy is more diffuse.	en
dc.format.extent	123215 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?2002ASPC..271..191L	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0112167	en
dc.rights	2002 Astronomical Society of the Pacific	en
dc.title	The Vela pulsar wind nebula at 6 cm	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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