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Supernovae pp 63-65 | Cite as

The Evolution of Supernova Remnants

  • John R. Dickel
  • D. C. Wells
  • T. R. Gull
  • A. G. Willis
  • S. van den Bergh
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 66)

Abstract

Recent advances in image tube photography and other optical techniques together with the opportunity to obtain high resolution radio maps, have now given us the ability to follow in detail the evolution in morphology of supernova remnants. To keep our summary of this evolution brief we shall limit our discussion to only two representative examples: the very young remnant of Tycho’s supernova and the much older remnant CTB1.

Keywords

Radio Emission Interstellar Medium Radio Galaxy Supernova Remnant Bright Radio 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Bergh, S. van den, Marscher, A. P. and Terzian, Y. 1973, Ap. J. Suppl., 26, 19.ADSCrossRefGoogle Scholar
  2. Dickel, J. R. and Milne, D. K. 1976, Austr. J. Phys., in press.Google Scholar
  3. Duin, R. M. and van der Laan, H. 1975, Astron. Astrophys., 40, 111.ADSGoogle Scholar
  4. Wells, D. C. 1975, in Proceedings of the Conference of Automation in Astronomy, Cambridge, Mass.Google Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht-Holland 1977

Authors and Affiliations

  • John R. Dickel
    • 1
  • D. C. Wells
    • 2
  • T. R. Gull
    • 3
  • A. G. Willis
    • 4
  • S. van den Bergh
    • 5
  1. 1.University of Illinois ObservatoryUSA
  2. 2.Kitt Peak National ObservatoryUSA
  3. 3.Lockheed Elec. CorporationUSA
  4. 4.Leiden SterrewachtNetherlands
  5. 5.David Dunlap ObservatoryCanada

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