A Comparison of Absorption- and Emission-Line Abundances in the Nearby Damped Lya Galaxy SBS 1543+593
Characterizing Transition Temperature Gas in the Galactic Corona
Damped Lya Absorption from the Nearby Low Surface Brightness Galaxy SBS 1543+593: a Summary
Emission-Line Spectroscopy of Damped Lya Systems: The Case of SBS 1543+593/HS 1543+5921
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Metallicity and Ionization in High-Velocity Cloud Complex C
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-08-10T11:32:23Z/2004-01-29T23:24:22Z
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, Bowen comma David V., 2007, 'The rarest of sightlines: probing the metallicity of a DLA with a nearby Low Surface Brightness galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-w3rd88f