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The bolometric luminosity function for the lowest mass stars

Published online by Cambridge University Press:  07 August 2017

Christopher G. Tinney
Christopher G. Tinney*
Affiliation:
California Institute of Technology, 105-24 Pasadena, CA 91125

Abstract

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We present a luminosity function (LF) for the coolest stars in three POSSII fields - extending earlier LFs to much lower masses at higher precision than has been acheived previously.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 496
Copyright
Copyright © Kluwer 

References

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