Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Lead, Tin, and Germanium in the Small Magellanic Cloud Main-Sequence B Star AV 304
The iron abundance of the Magellanic Bridge
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-03-27T05:28:07Z/1999-03-27T15:46:19Z
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, Peters et al., 2006, 'Heavy Element Abundances in AV 304, a B0.5 Main Sequence Star in the Small Magellanic Cloud', 1.0, European Space Agency, https://doi.org/10.5270/esa-0ywpr99