Analysis of the HST Ultraviolet Spectra for T Tauri Stars: RY Tau and HD115043
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Evidence of Stellar-driven Outflows from the Classical T Tauri Star RY Tau
Formation of Fe X-Fe XIV coronal lines in the accretion shock of 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
Resolving the Inner Arcsecond of the RY Tau Jet with HST
Instrument
HRS, HRS/2
Temporal Coverage
1993-12-31T04:20:35Z/1993-12-31T09:03:07Z
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., 1994, 'NON-RADIATIVE HEATING IN PRE-MAIN SEQUENCE STARS: CYCLE 3, HIGH PRIORITY', 1.0, European Space Agency, https://doi.org/10.5270/esa-upkjv18