Accuracy of element abundances from stellar atmospheres : proceedings of two sessions allocated at the IAU General Assembly in Baltimore, USA, August 1988 / R. Wehrse (ed.).
Contributor(s): Wehrse, R. (Rainer)
| International Astronomical Union. General Assembly (1988 : Baltimore, Md.)
Material type: 
TextSeries: Lecture notes in physics (Online): 356.Publisher: Berlin ; New York : Springer-Verlag, ©1990Description: 1 online resource (109 pages) : illustrationsContent type: text Media type: computer Carrier type: online resourceISBN: 9783540469711; 3540469710Subject(s): Stars -- Atmospheres | Stars -- Spectra | Cosmic abundances | Étoiles -- Atmosphères | Étoiles -- Spectre | Abondances cosmiques | Cosmic abundances | Stars -- Atmospheres | Stars -- Spectra | Sterren | Atmosfeer | Samenstelling | Spektralanalyse | Genauigkeit | Sternatmosphäre | Elementenhäufigkeit | Baltimore <Md., 1988>Genre/Form: Electronic books. Additional physical formats: Print version:: Accuracy of element abundances from stellar atmospheres.DDC classification: 523.8 LOC classification: QB809 | .A27 1990Other classification: 39.49 | 39.22 Online resources: Click here to access online Action note: digitized 2010 committed to preserveSummary: To get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.
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Title from PDF of title page (viewed Jun. 24, 2008).
Includes bibliographical references.
To get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.
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