High-Resolution Measurements of Intersystem Bands of Carbon Monoxide toward X Persei
Hubble Space Telescope Measurements of Vacuum Ultraviolet Lines of Interstellar CH
Hubble Space Telescope Survey of Interstellar 12CO/13CO in the Solar Neighborhood
Is There Enhanced Depletion of Gas-Phase Nitrogen in Moderately Reddened Lines of Sight?
Potential Variations in the Interstellar N I Abundance
The abundance of boron in diffuse interstellar clouds
The Abundance of Boron in Diffuse Interstellar Clouds
The Interstellar N/O Abundance Ratio: Evidence for Local Infall?
Ultraviolet Detection of Interstellar 12C17O and the CO Isotopomeric Ratios toward X Persei
Ultraviolet Measurements of Interstellar C2
Updated interstellar abundance studies and implications for dust models
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-10-27T08:30:53Z/2001-09-11T20:06:41Z
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, Lambert comma David L., 2006, 'The Interstellar Isotopic Ratio of Boron toward Omicron Persei and Nearby Sight Lines', 1.0, European Space Agency, https://doi.org/10.5270/esa-ur4mp7m