Fig. 4: Distributions of density, temperature, and metallicity.
From: Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind
Distributions of density and temperature at t = 360 + 19 Myr are presented in a and b, respectively. Both cavities inflated by nuclear outflow appear to tilt toward the CGM wind’s moving direction. Panel c presents the metallicity and velocity distribution at t = 360 + 19 Myr (the metallicities of both the nuclear outflow and the initial halo are set to be 0.5Z⊙). Panel d presents a 3D view of the density distribution. Coordinate values are in units of kpc.
