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The abundances of SN1987A

  • Novae, Supernovae, Supernova Remnants
  • Conference paper
  • First Online:
New Aspects of Magellanic Cloud Research

Part of the book series: Lecture Notes in Physics ((LNP,volume 416))

  • 138 Accesses

Abstract

The spectra of SN 1987A have been analyzed and modeled by various authors. However, in contrast to the other objects discussed in this volume there is not yet a comprehensive abundance analysis for this object. The reasons for this situation are manifold and depend on the expansion phase. We emphasize here the difficulties of spectral diagnostics during the coasting phase. Taking the resulting uncertainties into account we discuss some recent determinations of the composition.

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References

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Author information

Authors and Affiliations

  1. Institut für Theoretische Astrophysik, Im Neuenheimer Feld 561, D 6900, Heidelberg, Germany

    Rainer Wehrse

Authors
  1. Rainer Wehrse
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Editor information

Bodo Baschek Gerhard Klare James Lequeux

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© 1993 Springer-Verlag

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Wehrse, R. (1993). The abundances of SN1987A. In: Baschek, B., Klare, G., Lequeux, J. (eds) New Aspects of Magellanic Cloud Research. Lecture Notes in Physics, vol 416. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-56432-2_199

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  • DOI: https://doi.org/10.1007/3-540-56432-2_199

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-56432-4

  • Online ISBN: 978-3-540-47556-9

  • eBook Packages: Springer Book Archive

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