Accuracy of Element Abundances from Stellar Atmospheres Proceedings of Two Sessions Allocated at the IAU General Assembly in Baltimore, USA, August 1988
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...
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Format: | eBook |
Language: | English |
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Berlin, Heidelberg
Springer Berlin Heidelberg
1990, 1990
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Edition: | 1st ed. 1990 |
Series: | Lecture Notes in Physics
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Online Access: | |
Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- On the accuracy of atomic transition probabilities
- Accuracy of excitation and ionisation cross sections
- Accuracy of line broadening data
- Accuracy of abundances from O to mid B main sequence stars
- The accuracy of abundances from middle B to F main sequence normal stars
- Accuracy of the determination of the abundances in solar type stars
- Problems associated with cool dwarf stars
- Accuracy of abundances from stars in near-by galaxies