Emission of Kepler's Supernova Remnant Produced by Accelerated Cosmic Rays

Berezhko, Evgeni; Ksenofontov, Leonid; Völk, Heinrich

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Emission of Kepler's Supernova Remnant Produced by Accelerated Cosmic Rays

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Völk, Heinrich
Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society;

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引用

Berezhko, E., Ksenofontov, L., & Völk, H. (2005). Emission of Kepler's Supernova Remnant Produced by Accelerated Cosmic Rays. In J., Blümer (Ed.), Contributions to the 29th International Cosmic Ray Conference, Pune, India, 2005 (pp. 227-230). Karlsruhe: Forschungszentrum Karlsruhe.

引用: https://hdl.handle.net/11858/00-001M-0000-0011-876F-0

要旨

The nonlinear kinetic model of cosmic ray acceleration in supernova remnants (SNRs) is used to describe the properties of the Kepler's SNR. The calculated expansion law and the radio and X-ray emission produced by the accelerated cosmic rays in Kepler's SNR agree quite well with the observations. A rather large interior magnetic field about 200 μG is required to give a good fit for the radio and X-ray synchrotron emission. The predicted TeV gamma-ray emission, which is of hadronic origin, is expected at a detectable level.