Non-thermal insights on mass and energy flows through the Galactic Centre and into the Fermi bubbles
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Crocker, Roland
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Blackwell Publishing Ltd
Abstract
We construct a simple model of the star-formation- (and resultant supernova-) driven mass and energy flows through the inner ~200pc (in diameter) of the Galaxy. Our modelling is constrained, in particular, by the non-thermal radio continuum and γ-ray sig
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Monthly Notices of the Royal Astronomical Society
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Open Access
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