Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T07:34:24.127Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Reid, I.N. 1986, M.N.R.A.S. , 225, 873.CrossRefGoogle Scholar
Monet, D. et al. 1991, A.J., submitted.Google Scholar
Hawkins, M. & Bessell, M. 1988, M.N.R.A.S. , 234, 177.CrossRefGoogle Scholar