Constraints on the Ionization Balance of Hot-Star Winds from FUSE Observations of O Stars in the Large Magellanic Cloud
Effects of Metallicity on the Rotational Velocities of Massive Stars
Interstellar absorptions towards the LMC:. small-scale density variations in Milky Way disc gas
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
The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II l1640 in young star clusters
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1998-11-06T06:47:23Z/1998-11-15T09:27:10Z
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 comma Dominik J., 2007, 'Interfaces Between Hot and Cold Gas: The Superbubble N51D in the LMC', 1.0, European Space Agency, https://doi.org/10.5270/esa-56vswv3