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
New observations of NGC 1624-2 reveal a complex magnetospheric structure and underlying surface magnetic geometry
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-02-17T06:08:59Z/2015-10-06T18:24:42Z
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, Petit comma Veronique, 2016, 'Probing the extreme wind confinement of the most magnetic O star with COS spectroscopy', 1.0, European Space Agency, https://doi.org/10.5270/esa-ezay91s