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Energetic winds from low mass young stellar objects

  • Activity in Pre-Main Sequence Stars
  • Conference paper
  • First Online:
Cool Stars, Stellar Systems, and the Sun

Part of the book series: Lecture Notes in Physics ((LNP,volume 291))

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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.

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Authors and Affiliations

  1. Five College Astronomy Department, Smith College and the University of Massachusetts, 01063, Northampton, MA

    Suzan Edwards & Stephen E. Strom

Authors
  1. Suzan Edwards
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  2. Stephen E. Strom
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Editor information

Jeffrey L. Linsky Robert E. Stencel

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© 1987 Springer-Verlag

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Edwards, S., Strom, S.E. (1987). Energetic winds from low mass young stellar objects. In: Linsky, J.L., Stencel, R.E. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 291. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-18653-0_171

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  • DOI: https://doi.org/10.1007/3-540-18653-0_171

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-18653-3

  • Online ISBN: 978-3-540-48041-9

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