Line luminosities of Galactic and Magellanic Cloud Wolf-Rayet stars
Nitrogen line spectroscopy in O-stars. III. The earliest O-stars
Spectral classification of O2-3.5 If*/WN5-7 stars
Star Formation in R136: A Cluster of O3 Stars Revealed by Hubble Space Telescope Spectroscopy
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 Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars and Results from the Complete Sample
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150Msolar stellar mass limit
The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence
The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class
VLT-MAD observations of the core of 30 Doradus
Instrument
FOS/RD
Temporal Coverage
1996-11-11T20:34:12Z/1997-01-01T23:40:26Z
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, Massey comma Philip Louis, 1998, 'Star Formation in the Prototype Super Star Cluster R136', 1.0, European Space Agency, https://doi.org/10.5270/esa-m4ljl7q