Non-thermal insights on mass and energy flows through the Galactic Centre and into the Fermi bubbles
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
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Crocker_Non-thermal_insights_on_mass_2012.pdf||2.43 MB||Adobe PDF|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.