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The Evolution of Young Supernova Remnants

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Supernovae and Supernova Remnants

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 45))

Abstract

It has been shown (e.g. Woltjer, 1970) that many of the properties of a supernova remnant can be predicted from general considerations of the expansion of a massive gas cloud into the interstellar medium. However, this simple picture has been unable to explain the very powerful non-thermal radio emission from the young shell supernova remnants such as Cas A and 3C 10. In order to account for this it is necessary to invoke other mechanisms to produce magnetic field and relativistic particles.

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© 1974 D. Reidel Publishing Company, Dordrecht-Holland

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Gull, S.F. (1974). The Evolution of Young Supernova Remnants. In: Cosmovici, C.B. (eds) Supernovae and Supernova Remnants. Astrophysics and Space Science Library, vol 45. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2166-1_40

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  • DOI: https://doi.org/10.1007/978-94-010-2166-1_40

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-2168-5

  • Online ISBN: 978-94-010-2166-1

  • eBook Packages: Springer Book Archive

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