
doi: 10.1086/160326
A search for high-velocity moleular gas in the /sup 12/CO J = 1-0 transition around 28 T Tauri and three Herbig Ae/Be stars reveals high-velocity CO emission towrd T Tau, AS 353 A, and HL Tau. Maps of the spatially extended, high-velocity gas around T Tau and AS 353 A yield mass-loss rates of greater than 1 x 10/sup -7/ M/sub sun/ yr/sup -1/, respectively. These values are in excess of the 3 x 10/sup -8/ M/sub sun/ yr/sup -1/ theoretical limit set by DeCampli for mass-loss rates from T Tauri stars. The association of high-velocity CO wings with the presence of Herbig-Haro objects and the impact of T Tauri winds on molecular cloud dynamics are discussed.
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