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| Paper: |
Emission lines and winds from T Tauri stars |
| Volume: |
9, Cool Stars, Stellar Systems, and the Sun: Sixth Cambridge Workshop |
| Page: |
289 |
| Authors: |
Hartmann, L. |
| Abstract: |
Strong emission lines and excess optical continuum emission are only seen in T Tauri stars when a circumstellar disk is present, as indicated by IR excess emission. Thus, it appears that the extreme emission and winds of T Tauri stars are probably driven by disk accretion. |
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