Line luminosities of Galactic and Magellanic Cloud Wolf-Rayet stars
On the Evolutionary Phase and Mass Loss of the Wolf-Rayet--like Stars in R136a
Quantitative spectroscopy of Wolf-Rayet stars in HD97950 and R136a - the cores of giant HII regions
Radiation-driven winds of hot luminous stars XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters
Reduced Wolf-Rayet line luminosities at low metallicity
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150Msolar stellar mass limit
The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class
Instrument
HRS, HRS/1
Temporal Coverage
1994-07-28T14:15:41Z/1994-07-28T19:44:32Z
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, Ebbets comma Dennis, 1995, 'UV SPECTRA OF THE BRIGHTEST COMPONENTS OF R136', 1.0, European Space Agency, https://doi.org/10.5270/esa-t8gi6ne