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Energetic winds from low mass young stellar objects

  • Suzan Edwards
  • Stephen E. Strom
Activity in Pre-Main Sequence Stars
Part of the Lecture Notes in Physics book series (LNP, volume 291)

Abstract

The wind properties from low mass young stellar objects, including deeply embedded infrared sources, classical T Tauri stars and weak emission pre-main sequence stars (“naked” T Tauri stars) are reviewed. Wind diagnostics for these objects are described and wind properties such as ubiquity, morphology, and energetics are compared. Energetic winds are found only among those objects for which there is evidence for circumstellar disks. We offer the hypothesis that the presence of energetic winds and opaque circumstellar disks are linked, and that accretion of material from the disk may be the ultimate powering source for the wind.

Keywords

Mass Loss Rate Tauri Star Circumstellar Disk Young Stellar Object Cloud Core 
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

  • Suzan Edwards
    • 1
  • Stephen E. Strom
    • 1
  1. 1.Five College Astronomy DepartmentSmith College and the University of MassachusettsNorthampton

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