A ~ 40 Year Variability Cycle in the Luminous Blue Variable/Wolf-Rayet Binary System HD 5980?
Far Ultraviolet Spectroscopic Explorer Observations of a Supernova Remnant in the Line of Sight to HD 5980 in the Small Magellanic Cloud
Hubble Space Telescope Observations of the Luminous Blue Variable/W-R Eclipsing Binary System HD 5980
Hubble Space Telescope STIS Observations of the Wolf-Rayet Star HD 5980 in the Small Magellanic Cloud. II. The Interstellar Medium Components
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Observations of the early stages in the formation of an LBV shell
On the Nature of the LBV/WR Eclipsing Binary System HD 5980
The Photospheric Absorption Lines in the Ultraviolet Spectrum of the Multiple System HD 5980
Thermal Pressures in the Interstellar Medium away from Stellar Environments
Wind Structure and Luminosity Variations in the Wolf-Rayet/Luminous Blue Variable HD 5980
Wolf-Rayet stars in the Small Magellanic Cloud. II. Analysis of the binaries
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1999-05-06T18:13:30Z/2000-04-20T16:10:51Z
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, Koenigsberger comma Gloria, 2006, 'The Changing Wind Structure of the Erupting SMC WN/LBV system HD5980', 1.0, European Space Agency, https://doi.org/10.5270/esa-vnbd59d