Fig. 1: Schematic of the circumgalactic medium (CGM) wind model. | Nature Communications

Fig. 1: Schematic of the circumgalactic medium (CGM) wind model.

From: Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind

Fig. 1

The yellow areas represent the radio Loop I in the northern halo and the eROSITA bubbles (eRBs), and the orange region marks the North Polar Spur (NPS) as the brightest part of Loop I and the Northern eRB. The green areas (including the blue inside) are 2.3 GHz polarized radio lobes (PRLs). The blue areas mark the WMAP haze (WH) in 23–41 GHz52 and Fermi bubbles (FBs).

Back to article page