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Model Atmospheres and Chemistry
Published online by Cambridge University Press: 19 July 2016
Abstract
The limitations imposed on the accuracy of the abundance determination by the current status of the stellar atmosphere models are discussed. It is shown that the very high S/N ratio and resolution in spectroscopic observations require the new additional steps in stellar atmosphere modeling and in the line formation theory.
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- Setting the Stage
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- Copyright © Kluwer 1991