Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
Hubble Space Telescope spectroscopy of the Balmer lines in Sirius B*
Lya Absorption from Heliosheath Neutrals
Refining our Knowledge of the White Dwarf Mass-Radius Relation with HST Observations of Sirius-type Binaries
Sirius B Imaged in the Mid-infrared: No Evidence for a Remnant Planetary System
The Precataclysmic Binary HS 1136+6646 May Have a Companion
The Shocking Power Sources of LINERs
Instrument
STIS, STIS/CCD
Temporal Coverage
2004-02-06T13:57:13Z/2004-02-06T14:42:52Z
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, Barstow comma Martin, 2006, 'Verifying the White Dwarf Mass-Radius Relation with Sirius B', 1.0, European Space Agency, https://doi.org/10.5270/esa-n1jetsx