Steady-state hadronic gamma-ray emission from 100-MYR-old Fermi Bubbles
Fermi Bubbles are enigmatic γ-ray features of the Galactic bulge. Both putative activity (within few × Myr) connected to the Galactic center super-massive black hole and, alternatively, nuclear star formation have been claimed as the energizing source o
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal Letters|
|01_Crocker_Steady-state_hadronic_2014.pdf||129.41 kB||Adobe PDF|
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