A Survey of Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope Sight Lines through High-Velocity Cloud Complex C
Characterizing Transition Temperature Gas in the Galactic Corona
Cross-correlation of Lyman a absorbers with gas-rich galaxies
High-Velocity Cloud Complex C: Galactic Fuel or Galactic Waste?
Metallicity and Ionization in High-Velocity Cloud Complex C
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
The Galaxy Environment of O VI Absorption Systems
The Local Lya Forest. II. Distribution of H I Absorbers,Doppler Widths, and Baryon Content
The Local Lya Forest. I. Observations with the GHRS/G160M on the Hubble Space Telescope
The Search for Intergalactic Hydrogen Clouds in Voids
Instrument
HRS, HRS/2
Temporal Coverage
1997-01-09T13:21:02Z/1997-01-09T17:05:22Z
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, Wakker comma Bart P., 1998, 'THE METALLICITY OF HIGH-VELOCITY CLOUD COMPLEX C', 1.0, European Space Agency, https://doi.org/10.5270/esa-21lkagr