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.).

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Material type: Text

text

Media type:

computer

Carrier type:

online resource

ISBN:

9783540469711
3540469710

Subject(s): Additional physical formats: Print version:: Accuracy of element abundances from stellar atmospheres.DDC classification:

523.8 20

LOC classification:

QB809 .A27 1990

Other classification:

39.49
39.22

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Summary: 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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Item type	Current library	Collection	Call number	Status	Date due	Barcode	Item holds
eBook	e-Library	eBook LN Physics		Available

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Title from PDF of title page (viewed June 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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