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Spectroscopic Signatures of Microjets

Published online by Cambridge University Press:  25 May 2016

J. Solf
J. Solf*
Affiliation:
Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-77778 Tautenburg, FRG

Abstract

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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.

Type
I. Herbig-Haro Objects, H2 Flows and Radio Jets
Information
Symposium - International Astronomical Union , Volume 182: Herbig-Haro Flows and the Birth of Low Mass Stars , 1997 , pp. 63 - 72
Copyright
Copyright © Kluwer 1997 

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