A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds
Constraints on the Ionization Balance of Hot-Star Winds from FUSE Observations of O Stars in the Large Magellanic Cloud
HSTUV measurements of wind structure and velocities in Local Group OB stars
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Quantitative UV spectroscopy of early O stars in the Magellanic Clouds. The determination of the stellar metallicities
The Physics of Massive OB Stars in Different Parent Galaxies. I. Ultraviolet and Optical Spectral Morphology in the Magellanic Clouds
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
Ultraviolet Line Spectra of Metal-poor Star-forming Galaxies
UV Spectroscopy of Metal-Poor Massive Stars in the Small Magellanic Cloud
Instrument
FOS/BL
Temporal Coverage
1992-06-04T07:58:13Z/1992-11-12T10:08:47Z
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, Kudritzki comma Rolf-Peter, 1994, 'THE PHYSICS OF MASSIVE O-STARS IN DIFFERENT PARENT GALAXIES. THE MAGELLANIC CLOUDS - PART 1', 1.0, European Space Agency, https://doi.org/10.5270/esa-6epek5c