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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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