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The Self Absorption Curve Method for the Analysis of Emission Lines of Complex Ions as a Diagnostic of the Structure of Stellar Envelopes

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B[e] Stars

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 233))

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Abstract

A semi-empirical method has been developed to study the emission lines of ions with complex spectra such as Fe II and Ti II, formed in many sorts of stellar envelope. Information can be obtained notably about the excitation conditions, the column density and the dimensions of the line emitting region, without making detailed model dependent complex radiative transfer computations. This method is particularly useful in the study of B[e] star envelopes.

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References

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Author information

Authors and Affiliations

  1. Institut d’Astrophysique (CNRS), 98 bis Boulevard Arago, 75014, Paris, France

    M. Friedjung

Authors
  1. M. Friedjung
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Editor information

Editors and Affiliations

  1. Observatoire de Paris-Meudon, France

    Anne Marie Hubert

  2. Observatoire de Strasbourg, France

    Carlos Jaschek

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© 1998 Springer Science+Business Media Dordrecht

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Friedjung, M. (1998). The Self Absorption Curve Method for the Analysis of Emission Lines of Complex Ions as a Diagnostic of the Structure of Stellar Envelopes. In: Hubert, A.M., Jaschek, C. (eds) B[e] Stars. Astrophysics and Space Science Library, vol 233. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9014-3_6

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  • DOI: https://doi.org/10.1007/978-94-015-9014-3_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5080-9

  • Online ISBN: 978-94-015-9014-3

  • eBook Packages: Springer Book Archive

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