Central Stars of Planetary Nebulae in the Large Magellanic Cloud: A Far-Ultraviolet Spectroscopic Analysis
Comprehensive modelling of the planetary nebula LMC-SMP 61 and its WC-type central star
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
Hubble Space Telescope Observations of Planetary Nebulae in the Magellanic Clouds. VI. Cycles 4 and 5 Ultraviolet Spectroscopy Using the Faint Object Spectrograph
Multiwavelength Modeling the SED of Luminous Supersoft X-Ray Sources in Large Magellanic Cloud and Small Magellanic Cloud
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
Instrument
FOS/BL
Temporal Coverage
1995-03-20T08:42:56Z/1995-03-23T05:52:01Z
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, Dopita comma Michael Andrew, 1996, 'POST ASYMPTOTIC GIANT BRANCH EVOLUTION IN THE MAGELLANIC CLOUDS - SPECTROSCOPY: CYCLE 4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-waf5ii8