Abundances and Depletions of Neutron-capture Elements in the Interstellar Medium
Characterizing Transition Temperature Gas in the Galactic Corona
Does the Milky Way Produce a Nuclear Galactic Wind?
Do starburst winds escape? Insights from QSO absorption lines
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
Multiwavelength study of the distribution of neutral gas in and around galaxies and groups of galaxies
Probing the Intergalactic Medium/Galaxy Connection. V. On the Origin of Lya and O VI Absorption at z < 0.2
The abundance of boron in diffuse interstellar clouds
The Abundance of Boron in Diffuse Interstellar Clouds
The Chemical Properties of Low-redshift QSOs
The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-11-08T17:12:43Z/2004-07-29T06:32:19Z
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, Stocke comma John Thomas, 2006, 'Probing Outflowing Winds from the Galactic Center', 1.0, European Space Agency, https://doi.org/10.5270/esa-axlo5jo