A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds
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
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
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-09-02T14:41:20Z/2001-01-31T08:04:04Z
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, Massey comma Philip Louis, 2006, 'The Physical Parameters of the Hottest, Most Luminous Stars as a Function of Metallicity', 1.0, European Space Agency, https://doi.org/10.5270/esa-t4lr4hu