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Theoretical backgrounds for interpretation of spectroscopic observations

Published online by Cambridge University Press:  25 February 2014

P. Hadrava
P. Hadrava*
Affiliation:
Astronomical Institute, Academy of Sciences, Prague
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Abstract

The advantage of analysis of observed data using their fit with theoretical model of the directly observed quantities is shown as well as the need for simultaneous solution of all available data. Some particular problems of disentangling of stellar spectra and model atmospheres of component stars of multiple systems are discussed.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 64: Setting a New Standard in the Analysis of Binary Stars , 2013 , pp. 211 - 218
Copyright
© EAS, EDP Sciences, 2014

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