Bonn 2010 – wissenschaftliches Programm

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T: Fachverband Teilchenphysik

T 93: Gammaastronomie II

T 93.2: Vortrag

Dienstag, 16. März 2010, 17:05–17:20, HG XVII

Modeling the very high energy emission of Supernova remnants — •Iurii Sushch — Humboldt Universität

Supernova remnants (SNRs) are observed in all energy bands from the radio to the very high energy (VHE) TeV emission. The VHE emission can be modeled using existing radio and X-ray data of SNRs. The modeling of the VHE emission was done within an electronic scenario taking into account synchrotron emission of electrons and inverse Compton scattering on CMB photons. As a result of modeling the predicted VHE flux is calculated and its dependence on the magnetic field is shown.

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