An HST Archival Study of Galactic Interstellar Zinc and Chromium
High-Velocity, High-Excitation Neutral Carbon in a Cloud in the VELA Supernova Remnant
Hot subdwarf wind models with accurate abundances. I. Hydrogen dominated stars HD 49798 and BD+18deg 2647
Hubble Space Telescope Observations of Interstellar Lines in Three High-Latitude Stars
Interstellar Gas-Phase Abundances and Physical Conditions toward Two Distant High-Latitude Halo Stars
Interstellar Lines in HD 72127A and B: A Binary Star behind the VELA Supernova Remnant
Instrument
HRS, HRS/2
Temporal Coverage
1992-04-21T10:35:24Z/1992-05-30T10:00:00Z
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, Jenkins comma Edward B., 1993, 'ABUNDANCE ENHANCEMENTS IN HALO GAS', 1.0, European Space Agency, https://doi.org/10.5270/esa-f7xexyz