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Empirical GF-Determination from the Solar Spectrum

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Physics of Formation of FeII Lines Outside LTE

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 138))

Abstract

We test the reliability of Fe I and Fe II oscillator strengths determined empirically from optical solar lines by comparing fits of the observed line widths and line depths for various formation parameters.

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References

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Author information

Authors and Affiliations

  1. Sterrewacht “Sonnenborgh”, Utrecht, The Netherlands

    Robert J. Rutten

  2. Main Astronomical Observatory, Kiev, USSR

    Roman I. Kostik

Authors
  1. Robert J. Rutten
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  2. Roman I. Kostik
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Editor information

Editors and Affiliations

  1. Istituto di Astrofisica Spaziale (CNR), Frascati, Italy

    Roberto Viotti

  2. Osservatorio Astronomico di Capodimonte, Napoli, Italy

    Alberto Vittone

  3. Institut d’Astrophysique (CNRS), Paris, France

    Michael Friedjung

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© 1988 D. Reidel Publishing Company

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Rutten, R.J., Kostik, R.I. (1988). Empirical GF-Determination from the Solar Spectrum. In: Viotti, R., Vittone, A., Friedjung, M. (eds) Physics of Formation of FeII Lines Outside LTE. Astrophysics and Space Science Library, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4023-9_11

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  • DOI: https://doi.org/10.1007/978-94-009-4023-9_11

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8285-3

  • Online ISBN: 978-94-009-4023-9

  • eBook Packages: Springer Book Archive

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