On the source of dense outflows from T Tauri Stars. and III. Winds driven from the star-disc shear layer

Ana I. Gomez de Castro, Brigitta von Rekowski

Ultraviolet observations of classical T Tauri Stars (cTTSs) have shown that there is a hot (Te ~ 80,000 K) and dense (ne ~ 1e10 cm-3) component associated with the large scale jet.…