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Mean Colors and Effective Temperatures of K and M Dwarfs

Published online by Cambridge University Press:  12 April 2016

Robert F. Wing*
Affiliation:
Astronomy Department, Ohio State University, Columbus, Ohio 43210 U.S.A.

Extract

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Many applications of multicolor wideband photometry depend upon the existence of a table of mean colors, i.e. a listing of the average values of the color indices B–V, V–R, etc. for each spectral type. Such a table relates the observed colors of unreddened stars to their temperature classes and enables one to draw a reference line representing the main sequence on any color-color diagram.

Type
Session I: General Characteristics of Active Dwarfs
Copyright
Copyright © Reidel 1983

References

Boeshaar, P.C. 1976, Ph.D. thesis, Ohio State University.Google Scholar
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Keenan, P.C., and McNeil, R.C. 1976, An Atlas of Spectra of the Cooler Stars: Types G, K, M, S, and C, The Ohio State University Press.Google Scholar
Smak, J., and Wing, R.F. 1979, Acta Astron. 29, 187.Google Scholar
Wing, R.F. 1973, in Spectral Classification and Multicolour Photometry, ed. Fehrenbach, Ch. and Westerlund, B.E. (Reidel), p. 209.Google Scholar
Wing, R.F., and Yorka, S.B. 1979, in Spectral Classification of the Future, ed. McCarthy, M.F., Philip, A.G.D., and Coyne, G.V. (Vatican Observatory), p. 519.Google Scholar