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.
The code requires an ionizing spectral energy distribution (SED) and parameters describing the physical properties of the absorbing gas
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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.