Bonn 2010 – wissenschaftliches Programm

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T: Fachverband Teilchenphysik

T 94: Gammaastronomie III

T 94.2: Vortrag

Mittwoch, 17. März 2010, 14:15–14:30, HG VII

Diffuse gamma-ray emission model — •Andreas Hillert, Sabrina Casanova, and Werner Hofmann — MPI-K Heidelberg

The diffuse gamma-ray emission in our Galaxy is produced by electrons interacting mainly with radiation fields and protons which interact with ambient gas. By simulating a population of galactic sources, which accelerate protons and electrons, distributed according to the populations of supernova remnants and pulsars at radio wavelengths, we estimate the diffuse gamma-ray emission at GeV and TeV energies from intermediate and high latitudes above the Galactic Plane. We present here the predictions of our model.

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