Reanalysis of 2016 XMM-Newton and NuSTAR data confirms a strong variable ultra-fast outflow in IRAS 13224-3809 with velocities >0.2c, velocity-luminosity correlation, rapid flare response, and evidence favoring magnetic over radiative driving.
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Unveiling the dynamics of the ultra-fast outflow in IRAS 13224-3809 with X-ray spectroscopy
Reanalysis of 2016 XMM-Newton and NuSTAR data confirms a strong variable ultra-fast outflow in IRAS 13224-3809 with velocities >0.2c, velocity-luminosity correlation, rapid flare response, and evidence favoring magnetic over radiative driving.