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The Origin of the Magellanic Stream

  • Simon Wayte
Conference paper

Summary

New observations of the Magellanic Stream are used in a recent discrete ram-pressure theory which proposes that the signs of interaction in the Magellanic System point to a collision event some 2–4 × 108 years ago, and that the collisions between the inter-Cloud gas and a discrete halo produce the Magellanic Stream.

Keywords

Collision Event Negative Velocity Magellanic Cloud Velocity Resolution Narrow Component 
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.

References

  1. Morras, R. 1985, Astron. J. 90, 1801.ADSCrossRefGoogle Scholar
  2. Wright, M. C. H. 1979, Astrophys. J. 233, 35.ADSCrossRefGoogle Scholar
  3. Wright, M. C. H. 1979, Astrophys. J. 234, 27.ADSCrossRefGoogle Scholar

Copyright information

© Springer-Verlag New York, Inc. 1989

Authors and Affiliations

  • Simon Wayte
    • 1
  1. 1.Mt. Stromlo and Siding Spring ObservatoriesCanberraAustralia

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