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Chromospheric and coronal heating in a volume-limited sample of K dwarfs

  • D. H. Neff
Heating of Stellar Chromospheres and Coronae
Part of the Lecture Notes in Physics book series (LNP, volume 291)

Abstract

We compare the chromospheric and coronal emission levels in an essentially bias-free sample of K dwarfs. We find a rough power law relation between the normalized soft x-ray flux and the Mg H h + k flux, and we find further evidence of a minimum surface flux level for Mg H h + k emission in cool dwarfs.

Keywords

Surface Flux Radiation Loss Coronal Heating Disk Star Chromospheric Emission 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1987

Authors and Affiliations

  • D. H. Neff
    • 1
    • 2
  1. 1.JILA & Dept. of PhysicsUniv. of ColoradoBoulder
  2. 2.J. A. Bookbinder & J. L. LinskyJILA, Univ. of ColoradoBoulder

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