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Physical Input for the Determination of Stellar Abundances

Published online by Cambridge University Press:  19 July 2016

B. Gustafsson
B. Gustafsson*
Affiliation:
Stockholm Observatory∗, S-133 00 SALTSJÖBADEN, Sweden

Abstract

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The fundamental parameters and the physical modelling and data used in the analysis of high-resolution high S/N spectra of stars are discussed. Particular emphasis is led on recent developments in these respects and the importance of further improvements is stressed.

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. 333 - 343
Copyright
Copyright © Kluwer 1988 

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