The Vela Pulsar Wind Nebula at 6cm

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dc.creatorLewis, Dion
dc.creatorDodson, Richard
dc.creatorMcConnell, David
dc.creatorDeshpande, Avinash
dc.date2001-12-07
dc.date.accessioned2026-07-07T02:01:44Z
dc.date.available2026-07-07T02:01:44Z
dc.descriptionObservations using the Australia Telescope Compact Array at a wavelength of 6 cm have uncovered the radio counterpart to the compact X-ray nebula 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.
dc.description4 pages, 3 figures. To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0112167
dc.identifierhttp://arxiv.org/abs/astro-ph/0112167
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3861
dc.subjectAstrophysics
dc.titleThe Vela Pulsar Wind Nebula at 6cm
dc.typetext

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