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Abundance Determination in Stars: Some Pitfalls
Published online by Cambridge University Press: 12 July 2004
Abstract
The determination of stellar abundances is the most direct observational test for astronuclear physics. The reliability of such determinations depends on the quality of the observational data, but also critically on a correct understanding of all atmospheric processes as well as on fundamental atomic and molecular data. We illustrate this different aspects with several recent examples which served as a general introduction to the "round table" on this subject.
- Type
- Research Article
- Information
- European Astronomical Society Publications Series , Volume 11: The Future Astronuclear Physics , 2004 , pp. 67 - 73
- Copyright
- © EAS, EDP Sciences, 2004