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The chemical composition of main sequence stars in the Magellanic Clouds

  • I. D. Howarth
  • P. L. Dufton
  • A. Fitzsimmons
  • W. R. J. Rolleston
II. Early-Type Stars in Other Galaxies
Part of the Lecture Notes in Physics book series (LNP, volume 401)

Keywords

Theoretical Spectrum Atmospheric Parameter Main Sequence Star Metal Abundance Magellanic Cloud 
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

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  9. Shortridge, K., 1991. SERC Starlink Miscellaneous User Document, No. 1.Google Scholar

Copyright information

© Springer-Verlag 1992

Authors and Affiliations

  • I. D. Howarth
    • 1
  • P. L. Dufton
    • 2
  • A. Fitzsimmons
    • 2
  • W. R. J. Rolleston
    • 2
  1. 1.Department of Physics and AstronomyUniversity College LondonLondon
  2. 2.Department of Pure and Applied PhysicsQueens University of BelfastBelfastUnited Kingdom

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