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Stellar Photospheres: Success, Failure, Ambiguity, & Ambition

Published online by Cambridge University Press:  26 May 2016

David F. Gray
David F. Gray*
Affiliation:
Department of Physics & Astronomy University of Western Ontario

Abstract

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Models are compared with observations in several examples, including spectroscopic temperature measurement, irradiance variations, stellar rotation from line profiles, and velocity fields in stellar photospheres. A few key issues for investigations in the near future are suggested.

Type
Session E. Comparison with Observations
Information
Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 287 - 300
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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