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Properties of the Winds of T Tauri Stars

Name: Properties of the Winds of T Tauri Stars
Creator: Nuria Calvet
Keywords: 13. Climate action, 0103 physical sciences, 10. No inequality, 01 natural sciences

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1997Publisher:Springer NetherlandsJournal:Symposium - International Astronomical Union, volume 182, pages 417-432 (issn: 0074-1809,

Authors: Nuria Calvet;

doi: 10.1007/978-94-011-5608-0_34 , 10.1017/s0074180900061829

Properties of the Winds of T Tauri Stars

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Abstract

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.

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	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	28
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