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The Hayashi Line

  • Rudolf Kippenhahn
  • Alfred Weigert
Chapter
  • 379 Downloads
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

We have seen that convection can occur in quite different regions of a star. In this section we consider the limiting case of fully convective stars, i.e. stars which are convective in the whole interior from centre to photosphere, while only the atmosphere remains radiative.

Keywords

Main Sequence Interior Solution Hydrostatic Equilibrium Radiative Region Ionization Zone 
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 Berlin Heidelberg 1990

Authors and Affiliations

  • Rudolf Kippenhahn
    • 1
  • Alfred Weigert
  1. 1.GöttingenGermany

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