BAT99-9 - a WC4 Wolf-Rayet star with nitrogen emission: evidence for binary evolution?
Far Ultraviolet Spectroscopic Explorer Spectroscopy of the O VI Resonance Doublet in Sand 2 (WO)
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Reduced Wolf-Rayet line luminosities at low metallicity
Spectral analyses of WC stars in the LMC
Stellar and wind properties of LMC WC4 stars. A metallicity dependence for Wolf-Rayet mass-loss rates
The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of Evolution
The Structure of the Stratospheric Aerosol Layer in the Equatorial and South Polar Regions of Jupiter
WO-type Wolf-Rayet Stars: The Last Hurrah of Massive Star Evolution
Instrument
FOS/BL
Temporal Coverage
1994-09-26T08:14:53Z/1996-03-26T22:16:24Z
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, Hillier et al., 1997, 'CONSTRAINTS ON MASSIVE STAR EVOLUTION FROM CARBON AND OXYGEN ABUNDANCES IN LMC WC/WO STARS: CYCLE4HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-kw7lhyb