Clues on the Origin and Evolution of Massive Contact Binaries: Atmosphere Analysis of VFTS 352
Constraining the overcontact phase in massive binary evolution. I. Mixing in V382 Cyg, VFTS 352, and OGLE SMC-SC10 108086
HST/COS Spectra of the Wind Lines of VFTS 102 and 285
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-05-12T21:38:54Z/2015-05-22T19:05:18Z
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, Sana comma Hugues, 2016, 'UV spectroscopy of the most massive overcontact binary known to date: on the verge of coalescence ?', 1.0, European Space Agency, https://doi.org/10.5270/esa-ig4tysd