Abundances and Depletions of Neutron-capture Elements in the Interstellar Medium
A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity
A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
Broadened profiles of diffuse interstellar bands
Far-ultraviolet Dust Extinction and Molecular Hydrogen in the Diffuse Milky Way Interstellar Medium
Interstellar H2 toward HD 147888
Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2009-10-02T18:57:04Z/2011-03-22T15:41:57Z
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, Meyer comma David M., 2012, 'The Distance Dependence of the Interstellar N/O Abundance Ratio: A Gould Belt Influence?', 1.0, European Space Agency, https://doi.org/10.5270/esa-etu51kt