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The stellar temperature scale from angular diameters and flux distributions

Published online by Cambridge University Press:  25 May 2016

A.J. Booth
A.J. Booth*
Affiliation:
University of Sydney, School of Physics A28, NSW 2006, Australia

Abstract

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The current situation for the measurement of effective temperatures from interferometrically determined angular diameters and spectrophometry in the UV, visible and IR is considered. Accuracies and reliabilities of the resulting temperatures are assessed and coverage of stellar types is discussed.

Type
The Stellar Effective Temperature Scale
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 147 - 152
Copyright
Copyright © Kluwer 1997 

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