Cool, warm and hot outflows from CTTS: The FUV view of DG Tau
HST far-ultraviolet imaging of DG Tauri. Fluorescent molecular hydrogen emission from the wide opening-angle outflow
HST FUV C iv observations of the hot DG Tauri jet
Hubble Space Telescope/STIS Spectroscopy of the Optical Outflow from DG Tauri: Indications for Rotation in the Initial Jet Channel
Hubble Space Telescope STIS Spectroscopy of the Optical Outflow from DG Tauri: Structure and Kinematics on Subarcsecond Scales
Locating the Launching Region of T Tauri Winds: The Case of DG Tauri
Numerical simulations of stellar jets and comparison between synthetic and observed maps: clues to the launch mechanism
Physical properties of the jet from DG Tauri on sub-arcsecond scales with HST/STIS
Predicted rotation signatures in MHD disc winds and comparison to DG Tau observations.
The accretion/ejection paradigm of low mass stars tested with HST
The Ne III Jet of DG Tau and its Ionization Scenarios
Instrument
STIS, STIS/CCD
Temporal Coverage
1999-01-14T05:37:35Z/1999-01-14T17:03:17Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Mundt comma Reinhard, 2006, 'Spectroscopic Imaging of DG Tau -- Clues to the Structure and Collimation of T Tauri Star Winds', 1.0, European Space Agency, https://doi.org/10.5270/esa-u0fa7w6