A combined HST and XMM-Newton campaign for the magnetic O9.7 V star HD 54879. Constraining the weak-wind problem of massive stars
Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2016-04-30T03:36:29Z/2016-04-30T04:22:52Z
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, Hamann et al., 2017, 'Joint XMM-Newton and HST study of the magnetic weak-wind O-star HD 54879', 1.0, European Space Agency, https://doi.org/10.5270/esa-y9q7357