Extinction towards the cluster R136 in the Large Magellanic Cloud. An extinction law from the near-infrared to the ultraviolet
Massive Stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions
The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II l1640 in young star clusters
The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds
The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136
The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2012-04-04T15:22:55Z/2012-10-23T13:54:05Z
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, Crowther et al., 2013, 'A Massive Star Census of the Starburst Cluster R136', 1.0, European Space Agency, https://doi.org/10.5270/esa-57c3bok