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Luminosity Calibration of Giants and Supergiants, G0–M5

Published online by Cambridge University Press:  07 February 2017

Ph. C. Keenan*
Affiliation:
Perkins Observatory, The Ohio State and Ohio Wesleyan Universities, Ohio, U.S.A.

Abstract

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Calibration curves giving Mv for stars of luminosity classes III, II, Ib, Iab and 0 are derived and shown graphically in the HR diagram. There are serious gaps in which the calibration needs to be improved.

Type
Part III: Calibration of Spectroscopic Parallaxes
Copyright
Copyright © Reidel 1973 

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