The stellar content of nearby clouds — T Tauri stars

  • Claude Bertout
Part V: Stellar Content of Nearby Molecular Clouds
Part of the Lecture Notes in Physics book series (LNP, volume 237)


After a brief summary of the properties of T Tauri stars, we review current mass-loss rate determinations and line profile computations.


Radio Emission Line Profile Stellar Wind Tauri Star Balmer Line 
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 1985

Authors and Affiliations

  • Claude Bertout
    • 1
  1. 1.Laboratoire d'Astrophysique théorique du Collège de France and Institut d'AstrophysiqueParisFrance

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