Fig. 2: Simulated eRBs.
From: Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind
Panel a shows the simulated eRBs for the CGM wind model at t = 360 + 19 Myr. We masked the region of ∣Z∣ < 2 kpc. Edges of the observed NeRB and FBs are plotted in white line with diamonds (coordinate values are in Supplemental Note 1) and yellow dashed line14, respectively. The red crosses mark the bound of the observed PRLs15. Panels b, c, and d show the X-ray surface brightness profiles at b = ±40°, ±50°, and ±60°, respectively, in which the observed profiles16 for comparison are plotted with dashed lines.
