Blue Horizontal-Branch Stars in Old, Metal-rich Stellar Systems
CoolCAT
Detection of Neutral Phosphorus in the Near-ultraviolet Spectra of Late-type Stars
Germanium, Arsenic, and Selenium Abundances in Metal-poor Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Modeling Mid-Ultraviolet Spectra. I. Temperatures of Metal-poor Stars
Physical structure of the local interstellar medium
Searching for a gas cloud surrounding the WASP-18 planetary system
The Chemical Evolution of Phosphorus
The interstellar cloud surrounding the Sun: a new perspective
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The three-dimensional physical structure of the local interstellar medium
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
1997-10-15T06:43:30Z/1999-07-19T04:22:34Z
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.
