Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
Hubble Space Telescope FUV Spectra of the Post-common-envelope Hyades Binary V471 Tauri
Molecular hydrogen fluorescence and accretion in far-ultraviolet spectra of classical T Tauri stars
Revised Stellar Parameters for V471 Tau, A Post-common Envelope Binary in the Hyades
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
The age, life expectancy, and space density of Post Common Envelope Binaries
The Loopy Ultraviolet Line Profiles of RU Lupi: Accretion, Outflows, and Fluorescence
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-08-24T16:56:07Z/2000-09-02T12:30:21Z
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, Bond comma Howard E., 2006, 'Two Post-Common-Envelope Binaries in the Hyades Cluster', 1.0, European Space Agency, https://doi.org/10.5270/esa-5s04jz6