H II Regions in the Magellanic Clouds

  • G. Courtès
Conference paper

Summary

The H II regions are, in the LMC and SMC, a dominant phenomenon rich in various structures. The relative proximity of the Clouds offers an exceptional opportunity for detailed morphological and spectrographic observations. New results on kinematics and physics of the ionized interstellar medium are described. New directions for future observations are suggested.

Keywords

Dust Stratification Spectrophotometry CalI Peaked 

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Copyright information

© Springer-Verlag New York, Inc. 1989

Authors and Affiliations

  • G. Courtès
    • 1
  1. 1.Laboratoire d’Astronomie Spatiale du CNRS and Observatoire de MarseilleMarseilleFrance

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