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What do we do when models don't fit? On model atmospheres and real stellar spectra

Published online by Cambridge University Press:  25 May 2016

Bengt Gustafsson*
Affiliation:
Uppsala Astronomical Observatory Box 515, S-751 20 Uppsala, Sweden (Bengt. Gustafsson@astro.uu.se)

Abstract

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Developments in the modelling of stellar atmospheres and results from the confrontation between calculated and observed fluxes and spectra are discussed. It is argued that, although impressive advances in the study of O-type, WR and cool star spectra have recently occurred, significant improvements should be possible with already existing methods in the analysis of, e.g., solar-type stars.

Type
Stellar Atmospheres
Copyright
Copyright © Kluwer 1997 

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