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Accurate Spectroscopy of Intermediate and Late Spectral Types

Published online by Cambridge University Press:  19 July 2016

H. Holweger
H. Holweger*
Affiliation:
Institut für Theoretische Physik und Sternwarte der Universität Kiel, Olshausenstrasse 40, D-2300 Kiel, Federal Republic of Germany

Abstract

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Elemental abundances in the Sun and in meteorites are examined with respect to their qualification as a standard of population I composition. Some problems that arise in connection with spectroscopic determinations of abundances in the Sun, and in other late-type stars, are discussed with emphasis on photospheric models and departures from LTE.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 411 - 420
Copyright
Copyright © Kluwer 1988 

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