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A Note on the Calibration of Effective Temperatures

Published online by Cambridge University Press:  04 August 2017

J. R. W. Heintze
J. R. W. Heintze*
Affiliation:
“Sonnenborgh” Observatory, Utrecht

Abstract

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The discrepancy in the derived chemical compositions between B-Al stars and stars of later spectral types can be removed if another Teff-calibration is applied for A and F type stars than the one usually used.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 433 - 437
Copyright
Copyright © Reidel 1985 

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