Chandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rate
Dynamical Masses of Cool White Dwarfs in Double Degenerate Binary Systems
Measuring the Rotational Periods of Isolated Magnetic White Dwarfs
Radio observations of HD 93129A: The earliest O star with the highest mass loss?
Resolving OB Systems in the Carina Nebula with the Hubble Space Telescope Fine Guidance Sensor
The High Angular Resolution Multiplicity of Massive Stars
Instrument
FGS
Temporal Coverage
2002-03-12T09:03:10Z/2002-04-22T09:24:24Z
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, Nelan comma Edmund, 2002, 'A BEA Science Program: A High Angular Resolution Survey of Some of the Galaxy's Most Massive Stars', 1.0, European Space Agency, https://doi.org/10.57780/esa-7yqz131