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Recent observations of T Tauri stars

  • Suzan Edwards
  • Stephen E. Strom
1. Pre-Main Sequence Star
Part of the Lecture Notes in Physics book series (LNP, volume 193)

Abstract

The nature of the peculiar emission properties of the T Tauri stars is examined in the light of contributions from regions designated as photospheres, chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations of T Tauri activity can be linked to vigorous solar-stellar phenomena characteristic of cool stars of low mass, other characteristics of T Tauri behavior are exhibited by a wide range of young stellar objects.

Keywords

Mass Loss Rate Stellar Wind Stellar Surface Tauri Star Cool Star 
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 1984

Authors and Affiliations

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

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