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Transport processes in stellar interiors

  • Jean-Paul Zahn
Invited Reviews
Part of the Lecture Notes in Physics book series (LNP, volume 458)

Abstract

We first recall Evry Schatzman’s pioneering contributions to the theory of transport of matter and angular momentum in the radiative interior of stars. He suggested that this transport could be of turbulent nature and he linked it to the internal rotation state. We then review the major breakthroughs which have been accomplished during the eighties, mainly in the observational domain. Finally, we briefly describe some recent achievements on the theoretical side, and allude to the work in progress.

Keywords

Angular Momentum Internal Wave Differential Rotation Meridian Circulation Turbulent Transport 
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 1995

Authors and Affiliations

  • Jean-Paul Zahn
    • 1
    • 2
  1. 1.Département d’Astronomie Stellaire et Galactique, Observatoire de ParisSection de MeudonMeudonFrance
  2. 2.Astronomy DepartmentColumbia UniversityNew York

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