The Vela pulsar wind nebula at 6 cm
| 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.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.identifier.citation | ASP Conference Series, 2002, Vol.271, p191 | en |
| dc.identifier.uri | http://hdl.handle.net/2289/2669 | |
| 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 |