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- W4247741096 abstract "High-resolution long-slit spectroscopy of forbidden emission lines is used to investigate on a sub-arcsecond scale the spatial and kinematic properties and the physical conditions of the mass outflows from T Tauri stars in the immediate vicinity of the outflow source (microjets). Special attention is given to the case of DG Tau. The data permit us to distinguish physically different outflow components: (1) a high-velocity component (HVC) attributed to a fast jet, (2) a low-velocity component (LVC) attributed to gas entrained by the jet, and (3) a near-rest-velocity component (NRVC) attributed to a slow disk wind and/or disk corona." @default.
- W4247741096 created "2022-05-12" @default.
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- W4247741096 date "1997-01-01" @default.
- W4247741096 modified "2023-09-30" @default.
- W4247741096 title "Spectroscopic Signatures of Microjets" @default.
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- W4247741096 doi "https://doi.org/10.1017/s0074180900061544" @default.
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