A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
Ionization and Star Formation in the Giant H II Region SMC-N66
Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2018-12-23T20:47:56Z/2018-12-30T21:22:14Z
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, Oskinova comma Lidia, 2019, 'The low-metallicity starburst NGC346: massive-star population and feedback', 1.0, European Space Agency, https://doi.org/10.5270/esa-7702be9