Inferring the presence of very massive stars in local star-forming regions
Shining a Light on the Connections between Galactic Outflows Seen in Absorption and Emission Lines
Ultraviolet spectra of extreme nearby star-forming regions: Evidence for an overabundance of very massive stars
Very massive stars at low metallicity: Evolution, synthetic spectroscopy, and impact on the integrated light of starbursts
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2018-04-20T21:40:17Z/2019-02-01T03:30:53Z
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, Stark, 2019, 'Extreme Wolf-Rayet Galaxies with HST/COS: Understanding CIII] Emission in the Reionization Era', 1.0, European Space Agency, https://doi.org/10.5270/esa-0dvmx80