An HST Archival Study of Galactic Interstellar Zinc and Chromium
Atomic Physics with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. V. Oscillator Strengths for Neutral Carbon Lines below 1200 A
Dust in the Ionized Medium of the Galaxy: GHRS Measurements of AL III and S III
Highly Ionized Interstellar Atoms--Heated, Cooled, or Mixed?
High-Resolution Observations of Interstellar Ca I Absorption-Implications for Depletions and Electron Densities in Diffuse Clouds
High-Velocity Gas in GHRS Spectra of Three OB Stars
Interstellar Silicon Abundance
Nonthermal Chemistry in Diffuse Clouds with Low Molecular Abundances
Spatial and temporal variations in interstellar absorption towards HD 72127AB
The Amount of CH Produced during CH+ Synthesis in Interstellar Clouds
The Diffuse Interstellar Clouds toward 23 Orionis
The Interstellar Abundances of Tin and Four Other Heavy Elements
Variable Na I Absorption toward r Leonis: Biased Neutral Formation in the Diffuse Interstellar Medium?
Instrument
HRS, HRS/2
Temporal Coverage
1992-07-04T07:02:35Z/1992-12-11T23:22:41Z
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, Hobbs comma Lewis M., 1993, 'THE PROPERTIES OF SINGLE INTERSTELLAR CLOUDS: MODIFIED CYCLE 1 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-6hksh3n