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Calculations of line positions in the presence of magnetic and electric fields in white dwarf spectra

  • VII. Model Atmospheres and Radiative Transfer
  • Conference paper
  • First Online:
The Atmospheres of Early-Type Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 401))

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Abstract

We present first results of our line position calculations in the presence of strong magnetic and electric fields, as one can find in the dense atmospheres of magnetic White Dwarfs. The problem was solved by second order perturbation theory with hydrogenic wavefunctions calculated in a pure magnetic field and arbitrary orientations of the electric and magnetic fields.

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References

  • Tworz, J. (1989: private communication

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  • Zeller, G. (1990: PhD thesis, Fakultät für Physik der Universität Tübingen

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Authors and Affiliations

  1. Lehr- und Forschungsbereich Theoretische Astrophysik, Universität Tübingen, W-7400, Tübingen, Germany

    Susanne Friedrich & Hanns Ruder

  2. Landessternwarte, W-6900, Heidelberg, Germany

    Roland Östreicher

Authors
  1. Susanne Friedrich
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  2. Roland Östreicher
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  3. Hanns Ruder
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U. Heber C. Simon Jeffery

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© 1992 Springer-Verlag

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Friedrich, S., Östreicher, R., Ruder, H. (1992). Calculations of line positions in the presence of magnetic and electric fields in white dwarf spectra. In: Heber, U., Jeffery, C.S. (eds) The Atmospheres of Early-Type Stars. Lecture Notes in Physics, vol 401. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55256-1_346

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  • DOI: https://doi.org/10.1007/3-540-55256-1_346

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-55256-7

  • Online ISBN: 978-3-540-46997-1

  • eBook Packages: Springer Book Archive

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