Fe II emission lines in the UV spectrum of Sirius-A and VEGA
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
Ultraviolet observations of Sirius A and Sirius B with HST-GHRS. an interstellar cloud with a possible low deuterium abundance
UV Spectral Synthesis of Vega
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1996-08-28T05:37:34Z/1996-12-23T18:21:50Z
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, Vidal-Madjar comma Alfred, 1997, 'Far UV emission spectrum and stellar wind of Sirius A', 1.0, European Space Agency, https://doi.org/10.5270/esa-68932ju