A Compilation of Electronic Transitions in the CO Molecule and the Interpretation of Some Puzzling Interstellar Absorption Features
AL iii, SI iv, and C IV Absorption toward zeta Ophiuchi: Evidence for Photoionized and Collisionally Ionized Gas
An HST Archival Study of Galactic Interstellar Zinc and Chromium
A Statistical Equilibrium Analysis of Interstellar CO toward zeta Ophiuchi as Recorded by the Goddard High Resolution Spectrograph
A Weak Diffuse Interstellar Band in the Far-Ultraviolet Spectrum of zeta Ophiuchi
Dust in the Ionized Medium of the Galaxy: GHRS Measurements of AL III and S III
Fractionation of CO in the Diffuse Clouds toward zeta Ophiuchi
Interstellar Gas Phase Abundance of Carbon, Oxygen, Nitrogen, Copper, Gallium, Germanium, and Krypton toward zeta Ophiuchi
Interstellar TiII in the Milky Way and Magellanic Clouds
Revised chemical models of z Oph based on HST data
Scattered Light in the Echelle Modes of the Goddard High Resolution Spectrograph aboard the Hubble Space Telescope. II. Analysis of In-Flight Spectroscopic Observations
The Abundance of Mg in the Interstellar Medium
The Abundant Elements in Interstellar Dust
Time-Series Observations of O Stars. III. IUE and HST Spectroscopy of zeta Ophiuchi and Implications for the ``Photospheric Connection
Ultraviolet DIB at 1369 A Arising in Molecular Clouds
Ultraviolet Observations of the Gas Phase Abundances in the Diffuse Clouds toward zeta Ophiuchi at 3.5 Kilometers per Second Resolution
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1991-05-21T04:39:29Z/1991-05-22T01:38:36Z
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.
