Alternative model of stochastic cosmic ray acceleration by Rayleigh-Taylor instabilities in Fermi Bubbles shells to explain non-thermal halo emission.
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Uniform analysis of Suzaku, XMM-Newton, and Chandra data shows supersolar N/O and Ne/O in the warm-hot phase of the NPS and SPS, supporting their origin as limbs of Galactic bubbles.
citing papers explorer
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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.
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Thermal Structure and Chemical Enrichment of the North and South Polar Spurs: Supersolar N/O and Ne/O in the X-ray Plasma
Uniform analysis of Suzaku, XMM-Newton, and Chandra data shows supersolar N/O and Ne/O in the warm-hot phase of the NPS and SPS, supporting their origin as limbs of Galactic bubbles.