Cosmic rays and non-thermal emission in simulated galaxies – II. γ-ray maps, spectra, and the far-infrared–γ-ray relation

@inproceedings{Werhahn2021CosmicRA,
  title={Cosmic rays and non-thermal emission in simulated galaxies – II. $\gamma$-ray maps, spectra, and the far-infrared–$\gamma$-ray relation},
  author={Maria Werhahn and Christoph Pfrommer and Philipp Girichidis and Georg Winner},
  year={2021}
}
The γ-ray emission of star-forming (SF) galaxies is attributed to hadronic interactions of cosmic ray (CR) protons with the interstellar gas and contributions from CR electrons via bremsstrahlung and inverse Compton (IC) scattering. The relative importance of these processes in different galaxy types is still unclear. We model these processes in three-dimensional magnetohydrodynamical (MHD) simulations of the formation of isolated galactic discs using the moving-mesh code Arepo, including… 

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