Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T22:41:38.730Z Has data issue: false hasContentIssue false
  • English
  • Français

Statistics of Large Diameter Radio SNRs

Published online by Cambridge University Press:  13 May 2016

Abdul I. Asvarov
Abdul I. Asvarov*
Affiliation:
Institute of Physics, 33 H. Javid Ave, 370143 BAKU, Azerbaijan

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.

It is shown that if the recently discovered hypernova events are intrinsically energetic spherically symmetric explosions of massive stars than they can leave after themselves very large diameter (up to 500 pc) nonthermal radio shells with spectral properties like ordinary shell type radio supernova remnants (SNRs). The properties of such shells are modeled and compared with the statistics of large diameter SNRs.

Type
Supernovae, Pulsars, and the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 398 - 399
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Bell, A.R. 1978, MNRAS, 182, 443.CrossRefGoogle Scholar
Berkhuijsen, E.M. 1986, A&A, 166, 257.Google Scholar
Cox, D.P. & Anderson, P.R. 1982, ApJ, 253, 268.CrossRefGoogle Scholar
Duric, N., Gordon, S.M., Goss, W.M., et al., 1995, ApJ, 445, 173.CrossRefGoogle Scholar
Mathewson, D.S., Ford, V.L., Tuohy, I.R. et al. 1985, ApJS, 58, 197.CrossRefGoogle Scholar
Nomoto, K., Mazzali, P.A. & Nakamura, T. 2000 astro-ph, 0003077.Google Scholar