Alternative model of stochastic cosmic ray acceleration by Rayleigh-Taylor instabilities in Fermi Bubbles shells to explain non-thermal halo emission.
C R Acad Sci URSS
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Hydrodynamic model of nonthermal emission from the Fermi bubbles
Alternative model of stochastic cosmic ray acceleration by Rayleigh-Taylor instabilities in Fermi Bubbles shells to explain non-thermal halo emission.