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Note on Absolute Magnitudes in the Red and Infrared of Late M-Type Dwarfs

Published online by Cambridge University Press:  07 February 2017

S. L. Lippincott
S. L. Lippincott*
Affiliation:
Sproul Observatory, Swarthmore College, U.S.A.

Abstract

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The importance of red and infrared magnitudes for late dwarf M-type stars is stressed. The absolute magnitudes for the nearest stars with (R − I) ⩾ 1.20 is re-assessed.

Type
Part I: Absolute Magnitudes from Trigonometric and Statistical Parallaxes
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 18 - 20
Copyright
Copyright © Reidel 1973 

References

Kron, G. E., Gascoigne, S. C. B., and White, H. S.: 1957, Astron. J. 62, 205.CrossRefGoogle Scholar
Lippincott, S. L. and Hershey, J. L.: 1972, Astron. J. 77, 259.Google Scholar