Extended Data Fig. 4: Evolution of the outflow velocity and velocity width with precession phase.
From: Vertical wind structure in an X-ray binary revealed by a precessing accretion disk
Variation of the disk wind outflow velocity (top panel) and velocity width (bottom panel) versus the disk precession phase. Observations from the August 2020 XMM-Newton campaign are in black, archival XMM-Newton observations are in blue, and Chandra observations are in red color. Error bars indicate 1σ confidence intervals.
