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Abundance Effects in the Classification of K Stars

Published online by Cambridge University Press:  14 August 2015

P. M. Williams
P. M. Williams*
Affiliation:
Royal Observatory, Edinburgh, United Kingdom

Abstract

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The influence of metal abundance and gravity on the relation between spectral type and effective temperatures of late G and K type stars is investigated and calibrated using metal abundances from narrow-band photometry, near infrared photometry and independent luminosity estimates.

Type
Part III/Derivation of Abundances Through Photometric and Spectroscopic Methods
Information
Symposium - International Astronomical Union , Volume 72: Abundance Effects in Classification , 1976 , pp. 87 - 90
Copyright
Copyright © Reidel 1976 

References

Głebocki, R.: 1972, Acta Astron. 22,141.Google Scholar
Johnson, H. L. and Morgan, W. W.: 1953, Astrophys. J. 117, 313.CrossRefGoogle Scholar
Morgan, W. W.: 1937, Astrophys J. 85, 380.Google Scholar
Pannekoek, A.: 1922, Bull. Astron. Inst. Neth. 1, 107.Google Scholar
Roman, N. G.: 1952, Astrophys. J. 116, 122.Google Scholar
Williams, P. M.: 1971, Monthly Notices Roy. Astron. Soc. 153, 171.Google Scholar
Williams, P. M.: 1972, Monthly Notices Roy. Astron. Soc. 158, 361.Google Scholar