The accretion-ejection connexion in T Tauri stars: jet models vs. observations

Details The accretion-ejection connexion in T Tauri stars: jet models vs. observations The accretion-ejection connexion in T Tauri stars: jet models vs. observations

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..243..203c&link_type=abstract

Star-Disk Interaction in Young Stars, Proceedings of the International Astronomical Union, IAU Symposium, Volume 243, p. 203-214

Astronomy and Astrophysics

Astronomy

19

Hydrodynamics, Stars: Pre–Main-Sequence, Stars: Winds, Outflows, Ism: Jets And Outflows

Scientific paper

Key observational constraints for jet models in T Tauri stars are outlined, including the jet collimation scale, kinematic structure, and ejection/accretion ratio. It is shown that MHD self-collimation is most likely required. The four possible MHD ejection sites (stellar surface, inner disk edge, extended disk region, magnetosphere-disk reconnexion line) are then critically examined against observational constraints, and open issues are discussed.

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