Hot Evolved Objects in Different Parent Galaxies: The Stellar Winds of Three Planetary Nebula Nuclei in the Large Magellanic Cloud
Hubble Space Telescope observations of Magellanic cloud planetary nebulae: Stellar winds
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
WO-type Wolf-Rayet Stars: The Last Hurrah of Massive Star Evolution
Instrument
FOS/BL
Temporal Coverage
1994-11-16T08:57:55Z/1995-04-15T05:40:52Z
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 comma D. John, 1996, 'CONSTRAINTS ON MASSIVE STAR EVOLUTION FROM CARBON AND OXYGEN ABUNDANCES IN LMC WC STARS', 1.0, European Space Agency, https://doi.org/10.5270/esa-2zswf1b