Hubble Space Telescope Observations of Chromospheres in Metal-Deficient Field Giants
Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
New Abundance Determinations of Cadmium, Lutetium, and Osmium in the r-process Enriched Star BD +17 3248
New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars
The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
The Extremely Metal-poor, Neutron Capture-rich Star CS 22892-052: A Comprehensive Abundance Analysis
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
1999-05-24T23:26:52Z/2000-12-29T07:35:18Z
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, Sneden comma Christopher, 2007, 'CS 22892--052: A Rosetta Star for the Age and Early History of the Galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-6b86nxj