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Observations of the H and C recombination lines toward NGC 2024

  • T.L. Wilson
Part I: Molecular Clouds and Dust Clouds
Part of the Lecture Notes in Physics book series (LNP, volume 42)

Abstract

This report deals with radio observations of the carbon and narrow hydrogen recombination lines. The theoretical discussion of these data are contained in the paper by Walmsley, in this volume.

Keywords

Radial Velocity Line Emission Velocity Difference Theoretical Discussion Recombination Line 
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

  1. MacLeod, J.M., Doherty, L.H., Higgs, L.A., 1975, Astron. Astrophys., in press.Google Scholar
  2. Pedlar, A., Hart, L., 1974, Mon. Not. R. astron. Soc., 168, 577.Google Scholar
  3. Rickard, L.J., Zuckerman, B., Palmer, P., Turner, B.E., 1975, in prep.Google Scholar
  4. Wilson, T.L., Thomasson, P., Gardner, F.F., 1975, Astron. Astrophys., in press.Google Scholar
  5. Zuckerman, B., Ball, J., 1974, Astrophys. J., 190, 35.Google Scholar

Copyright information

© Springer-Verlag 1975

Authors and Affiliations

  • T.L. Wilson
    • 1
  1. 1.Max-Planck-Institut für RadioastronomieBonnGermany

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