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Non-thermal insights on mass and energy flows through the Galactic Centre and into the Fermi bubbles

Crocker, Roland


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

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1111/j.1365-2966.2012.21149.x


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