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Properties of the Winds of T Tauri Stars

Published online by Cambridge University Press:  25 May 2016

Nuria Calvet
Nuria Calvet*
Affiliation:
Centro de Investigaciones de Astronomía, Mérida, Venezuela, and Center for Astrophysics, 160 Concord, MA 02138, USA

Abstract

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The properties of Classical T Tauri (TTS) winds - their mass loss rate, temperature, origin, and energetics - are reviewed and interpreted in terms of the most recent observational evidence. TTS winds seem to have their origin in the disk and are powered by accretion. Most TTS have Ṁω ≤ 10–9Mʘ yr–1 and Ṁω/Ṁ ∼ 0.1, with T ∼ 104K.

Type
IV. Disks, Winds, and Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 182: Herbig-Haro Flows and the Birth of Low Mass Stars , 1997 , pp. 417 - 432
Copyright
Copyright © Kluwer 1997 

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