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Non-LTE analyses of B stars

  • Sylvia R. Becker
I. “Normal” Early-Type Stars
Part of the Lecture Notes in Physics book series (LNP, volume 401)

Abstract

In this paper we present a spectroscopic method for parameter determination in B stars and applications thereof. The derived abundances are considered in the context of the existence or non-existence of a radial gradient of galactic abundances.

Keywords

Monthly Notice Line Ratio Dielectronic Recombination Galactocentric Distance Ionisation Stage 
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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Copyright information

© Springer-Verlag 1992

Authors and Affiliations

  • Sylvia R. Becker
    • 1
  1. 1.Institut für Astronomie und Astrophysik der Universität MünchenMünchen 80Germany

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