Quantitative spectroscopy of Wolf-Rayet stars in HD97950 and R136a - the cores of giant HII regions
The Dense Galactic Starburst NGC 3603. I. HST/FOS Spectroscopy of Individual Stars in the Core and the source of Ionization and Kinetic Energy
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150Msolar stellar mass limit
Instrument
FOS/RD
Temporal Coverage
1994-09-05T02:20:06Z/1994-09-06T09:05:56Z
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, Drissen et al., 1995, 'THE STELLAR CONTENT AND DYNAMICS OF THE DENSE GALACTIC STARBURST NGC 3603: CYCLE4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-mz1nez2