Figure 2 (IMAGE)
Caption
Figure 2. Gamma-ray image of the Fermi bubbles (blue) overlaid on a map of RR Lyrae stars (red) observed by the GAIA telescope. The shape and orientation of the Sagittarius (Sgr) dwarf match perfectly well those of the Fermi cocoon – a bright substructure of gamma-ray radiation in the southern part of the Fermi bubbles. This is strong evidence that the Fermi cocoon is due to energetic processes occurring in Sagittarius, which from our perspective, is located behind the Fermi bubbles.
Credit
Crocker, Macias, Mackey, Krumholz, Ando, Horiuchi et al. (2022)
Usage Restrictions
Use credit
License
Original content