An Empirical Isochrone of Very Massive Stars in R136a
HSTUV measurements of wind structure and velocities in Local Group OB stars
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
Reduced Wolf-Rayet line luminosities at low metallicity
The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. I. A Sample of 20 Stars in the Magellanic Clouds
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150Msolar stellar mass limit
The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution
The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class
Instrument
FOS/RD, HRS, HRS/1, WFPC2, WFPC2/PC
Temporal Coverage
1996-01-31T15:16:15Z/1996-02-01T10:43:16Z
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, HEAP SARA R., 1997, 'READING THE ''ROSETTA STONE'': GHRS SPECTROSCOPY OF INDIVIDUAL STARS IN R136A', 1.0, European Space Agency, https://doi.org/10.5270/esa-09sz30t