Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-27T00:37:43.451Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio observations of SN 1006

Published online by Cambridge University Press:  01 August 2006

Estela M. Reynoso
Estela M. Reynoso*
Affiliation:
Instituto de Astronomía y Física del Espacio, C.C. 67, Suc. 28, 1428 Buenos Aires, Argentina email: [email protected]
*
†Member of the Carrera del Investigador Científico of CONICET, Argentina.
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this article I review our present knowledge of SN 1006 based on radio observations since the identification of the radio remnant four decades ago. I also report preliminary results of a new radio expansion study which combines VLA 1991/92 data with new VLA and ATCA observations performed in 2003.

Keywords

(ISM:) supernova remnantsindividual: SN 1006radio continuum: ISMradio lines: ISMpolarization
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 305
Copyright
Copyright © International Astronomical Union 2007

References

Dubner, G. M., Giacani, E. B., Goss, W. M., Green, A. J., & Nyman, L.-Å. 2002, A&A, 387, 1047Google Scholar
Dwarkadas, V. V., & Chevalier, R. A. 1998, ApJ, 497, 807CrossRefGoogle Scholar
Gardner, F. F., & Milne, D. K. 1965, AJ, 70, 754CrossRefGoogle Scholar
Moffett, D. A., Goss, W. M., & Reynolds, S. P. 1993, AJ, 106, 1566CrossRefGoogle Scholar
Reynolds, S. P., & Gilmore, D. M. 1993, AJ, 106, 272CrossRefGoogle Scholar