On the source of dense outflows from T Tauri stars - II. Warm disc winds
Recent ultraviolet (UV) observations suggest that there is a hot (T e ≃ 80000 K) and dense (Ne ≃ 1010 cm -3) wind associated with the large-scale jets observed in classical T Tauri stars (cTTSs). The observations of these rather evolved sources cannot be fitted with the classical cold disc wind solu...
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| Autores principales: | De Gómez Castro, A.I., Ferro-Fontán, C. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v362_n2_p569_DeGomezCastro |
| Aporte de: |
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