Turbulence in main sequence stars

  • Thomas Gehren
2. Observed Properties of Stellar Turbulence
Part of the Lecture Notes in Physics book series (LNP, volume 114)


Convection Zone Line Strength Main Sequence Star Microturbulence Velocity Small Scale Velocity 
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 1980

Authors and Affiliations

  • Thomas Gehren
    • 1
  1. 1.Max-Planck-Institut für AstronomieHeidelbergGermany

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