Effects of Metallicity on the Rotational Velocities of Massive Stars
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. II. Variations of Interstellar Depletions and Dust-to-gas Ratio within the LMC
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Properties and Origin of the High-Velocity Gas Toward the Large Magellanic Cloud
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-04-14T13:05:26Z/2000-04-14T17:05:21Z
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, Bomans et al., 2006, 'The H_2/CO ratio in the Large Magellanic Cloud', 1.0, European Space Agency, https://doi.org/10.5270/esa-ezru20s