Analysis of HST Ultraviolet Spectra for T Tauri Stars: RU Lup
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Hot Gas Lines in T Tauri Stars
Intercombinational Line Profiles in the UV Spectra of T Tauri Stars and Analysis of the Accretion Zone
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
New Constraints on Protostellar Jet Collimation from High-Density Gas UV Tracers
Observations of T Tauri Stars using Hubble Space Telescope GHRS. I. Far-Ultraviolet Emission Lines
Observations of T Tauri Stars Using the Hubble Space Telescope GHRS. II. Optical and Near-Ultraviolet Lines
The Loopy Ultraviolet Line Profiles of RU Lupi: Accretion, Outflows, and Fluorescence
Instrument
HRS, HRS/2
Temporal Coverage
1992-08-24T03:13:35Z/1992-08-24T06:31:28Z
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, Walter comma Frederick M., 1993, 'NON-RADIATIVE HEATING IN PRE-MAIN SEQUENCE STARS: CYCLE 2 CONTINUATION', 1.0, European Space Agency, https://doi.org/10.5270/esa-zuaql2c