Institute for Astrophysics and Computational Sciences
XRISM/Resolve observations of NGC 3516 provided the first intra-observation variability detection in highly ionized X-ray absorbers, constraining gas density to >10^6 cm^-3 and distance to <11.6 light days for one outflow. The study identified eight distinct photoionized gas components, including a transient ultra-fast inflow at ~14,800 km/s, and found a 40 ks oscillatory "rocking" motion in the Fe Kα emission correlated with continuum flux.
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