Interstellar Krypton Abundances: The Detection of Kiloparsec-scale Differences in Galactic Nucleosynthetic History
Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead
Probing the Role of Carbon in Ultraviolet Extinction along Galactic Sight Lines
The abundance of boron in diffuse interstellar clouds
The Abundance of Boron in Diffuse Interstellar Clouds
The Variation of Magnesium Depletion with Line-of-Sight Conditions
Updated interstellar abundance studies and implications for dust models
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-08-08T15:35:22Z/2004-02-20T11:25:58Z
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, Cartledge comma Stefan I. B., 2005, 'Exploring Interstellar Krypton Abundance Variations at Kiloparsec Scales', 1.0, European Space Agency, https://doi.org/10.5270/esa-flm9416