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

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.

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 Creators:
Berezhko, Evgeni1, Author
Ksenofontov, Leonid1, Author
Völk, Heinrich2, Author           
Affiliations:
1Yu.G.Shafer Institute of Cosmophysical Research and Aeronomy, 31 Lenin Ave., 677980 Yakutsk, Russia, ou_persistent22              
2Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: Supernova Remnant
 Abstract: 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.

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Language(s): eng - English
 Dates: 2005-12
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 277788
URI: http://icrc2005.tifr.res.in/
 Degree: -

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Title: 29th International Cosmic Ray Conference
Place of Event: Pune, India
Start-/End Date: 2005-08-03 - 2005-08-10

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Title: Contributions to the 29th International Cosmic Ray Conference, Pune, India, 2005
Source Genre: Proceedings
 Creator(s):
Blümer, Johannes, Editor
Affiliations:
-
Publ. Info: Karlsruhe : Forschungszentrum Karlsruhe
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 227 - 230 Identifier: -