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
Hubble Space Telescope Images of Magellanic Cloud Planetary Nebulae
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1998-12-30T11:36:24Z/1999-01-07T03:50:50Z
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, Hamann comma Wolf-Rainer, 2006, 'UV Spectroscopy of Wolf-Rayet-Type Central Stars in the Magellanic Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-l3ax2xb