Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Constraints to the magnetospheric properties of T Tauri stars - I. The C II, Fe II and Si II ultraviolet features
CoolCAT
How Hot is the Wind from TW Hydrae?
HST/COS Spectra of DF Tau and V4046 Sgr: First Detection of Molecular Hydrogen Absorption Against the Lyman a Emission Line
HST/COS Spectra of DF Tau and V4046 Sgr: First Detection of Molecular Hydrogen Absorption Against the Lya Emission Line
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Molecular hydrogen fluorescence and accretion in far-ultraviolet spectra of classical T Tauri stars
The Origins of Fluorescent H2 Emission From T Tauri Stars
UV Excess Measures of Accretion onto Young Very Low Mass Stars and Brown Dwarfs
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-09-18T20:06:27Z/1999-09-18T22:22:06Z
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, Linsky comma Jeffrey L., 2000, 'Accretion and Winds in T Tauri Systems', 1.0, European Space Agency, https://doi.org/10.5270/esa-w7x9fy3