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The 1s 2s states of negative hydrogen

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Abstract

Term values for the 1s 2s states of H− are calculated with the use of simple eigenfunction approximations constructed on the basis of available Hartree-type functions for the 1s 2 and 2s 2 states of the ion. The results seem to support a tentative identification of the interstellar diffuse absorption bands at λ4890 and λ6180 as due to negative hydrogen.

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References

  • Hartree, D. R.: 1957,The Calculation of Atomic Structures, Chapman-Hall and John Wiley, London and New York.

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  • Holöien, E.: 1958,Proc. Phys. Soc. (London)71, 357.

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  • Ingemann-Hilberg, C.: 1970, to be published.

  • Rudkjøbing, M.: 1969a,Astrophys. Space Sci. 3, 102.

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  • Rudkjøbing, M.: 1969b,Astrophys. Space Sci. 5, 68.

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Authors and Affiliations

  1. Computing Center, University of Aarhus, Denmark

    Claus Ingemann-Hilberg

  2. Ole Roemer Observatory, University of Aarhus, Denmark

    Mogens Rudkjøbing

Authors
  1. Claus Ingemann-Hilberg
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  2. Mogens Rudkjøbing
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Ingemann-Hilberg, C., Rudkjøbing, M. The 1s 2s states of negative hydrogen. Astrophys Space Sci 6, 101–106 (1970). https://doi.org/10.1007/BF00653621

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  • DOI: https://doi.org/10.1007/BF00653621

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