An HST Archival Study of Galactic Interstellar Zinc and Chromium
Dust in the Ionized Medium of the Galaxy: GHRS Measurements of AL III and S III
First Results from the Goddard High-Resolution Spectrograph: C i, S i, and CO toward XI Persei and the Physical Conditions in Diffuse Clouds
First Results from the Goddard High-Resolution Spectrograph: Element Abundances as a Function of Velocity in the Neutral Gas toward XI Persei
Goddard High-Resolution Spectrograph Observations of Narrow Discrete Stellar Wind Absorption Features in the Ultraviolet Spectrum of the O7.5 III Star XI Persei
Interstellar Silicon Abundance
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
Ultraviolet DIB at 1369 A Arising in Molecular Clouds
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1991-01-30T04:34:37Z/1991-01-30T20:57:40Z
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, Ebbets comma Dennis, 1991, 'XI PER INTERSTELLAR SPECTRUM GHRS SAT AND/OR ERO (PART II)', 1.0, European Space Agency, https://doi.org/10.5270/esa-8145myo
