Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/2669
Title: | The Vela pulsar wind nebula at 6 cm |
Authors: | Lewis, D. Dodson, R. McConnell, D. Deshpande, A.A. |
Issue Date: | 2002 |
Publisher: | Astronomical Society of the Pacific |
Citation: | ASP Conference Series, 2002, Vol.271, p191 |
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. |
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. |
URI: | http://hdl.handle.net/2289/2669 |
Alternative Location: | http://adsabs.harvard.edu/cgi-bin/bib_query?2002ASPC..271..191L http://arxiv.org/abs/astro-ph/0112167 |
Copyright: | 2002 Astronomical Society of the Pacific |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2002 ASP Conference V271 191p.pdf Restricted Access | Restricted Access | 120.33 kB | Adobe PDF | View/Open Request a copy |
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