Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
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
No breakdown of the radiatively driven wind theory in low-metallicity environments
Quantitative Studies of the Far-Ultraviolet, Ultraviolet, and Optical Spectra of Late O- and Early B-Type Supergiants in the Magellanic Clouds
Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. I. A Sample of 20 Stars 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
Instrument
FOS/BL
Temporal Coverage
1994-02-07T22:55:28Z/1995-03-12T00:06:37Z
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, Robert comma Carmelle, 1996, 'A UV SPECTRAL LIBRARY OF METAL-POOR MASSIVE STARS', 1.0, European Space Agency, https://doi.org/10.5270/esa-wnx6f9x